Journal of Oil, Gas and Petrochemical Sciences (JOGPS)

Open Access Journal

Frequency: Bi-Monthly

ISSN 2630-8541

Volume : 2 | Issue : 2

Research

Wellbore instability prediction and performance analysis using Poroelastic modeling

Dr. Ing Mohamed Halafawi,1 Dr. Ing Lazăr Avram2

1Doctor and Inginer, Petroleum-Gas University of Ploiesti, Romania
2Professor; Drilling, Extraction, and Transportation of Hydrocarbons, Petroleum-Gas University of Ploiesti, Romania

Received: April 18, 2019 | Published: July 11, 2019

Correspondence: Dr. Ing Mohamed Halafawi, Doctor and Inginer, Petroleum-Gas University of Ploiesti, Romania, Email: [email protected]

Citation: Halafawi DIM, Avram DIL. Wellbore instability prediction and performance analysis using Poroelastic modeling. J Oil Gas Petrochem Sci. (2019);2(2):93-106. DOI:10.30881/jogps.00028

Abstract

Wellbore instability problems give rise to increasing the non-productive time (NPT) and the non-productive cost while drilling tectonically stressed and unstable formations. In this article, a wellbore stability model is developed for predicting the behavior of borehole instability zones and the optimum wellbore trajectory which has the safest mud window with time. Geo-Mechanical Earth Model (MEM) was combined with failure criterion using logging while drilling /measurement while drilling (LWD/MWD) or wire line logging data as well. The developed model is generated iteratively in order to predict the optimum mud window and wellbore trajectory variations with time. The radial and tangential stress concentrations around the wellbore are determined using the poroelastic constitutive model. This model enables to take into consideration the effect of the rock pore structure. Failure criteria considering the intermediate stress are also used as the shear failure criterion. Additionally, the model provides more precise solutions to optimize the drilling fluids in this high tectonic area. The model is applied and verified in a deviated wellRBS-91 in which exist excessive mechanical wellbore breakouts while drilling the 8.5” hole section. The developed model shows a good results in predicting the wellbore instability compared with the actual wellbore images for instability zones (3650 m – 3800 m). For a long time period (30 hrs) after drilling this zone, the developed model shows that the maximum shear stress around the wellbore is at 63º and 243º counterclockwise which agree with the image logs. The safe pressure window is very narrow at the high deviation angle at the current well azimuth (240º). The minimum and maximum safe mud weight in order to avoid shear and tensile failure are found 9.8 and 15.5 ppg respectively. This well section obviously cannot be drilled horizontally in direction of the minimum horizontal stress (Azimuth = 60º) due to the narrow allowable mud window.

Keywords: Wellbore stability models, failure criteria, instability prediction, safe mud weight, optimum well trajectory

Introduction

Borehole instability is described as an undesirable state of an open hole interval that does not maintain its gauge size and shape and/or its structural integrity. Instability causes are divided into three categories:1-4 Mechanical (due to in-situ stresses), Erosion (due to fluid circulation), and Chemical (due to interaction of borehole fluid with the formation).Borehole instability gives rise to problems in drilling operations and design procedures. Instability problems produces non-productive time and sometimes also loss of equipment which means additional non-productive costs. Instability problems can appear in both vertical deviated and horizontal wells. Long extended reach deviated wells are especially known for having instability problems. Wells stability evaluation represents a rock mechanics problem which means prediction of a rock’s response to mechanical loading.1-3,5 Some special circumstances that make evaluation of stability problematic: 1-3,5

  • No methods available for direct observation of what is happening for the drill bit when it is several thousand of meters away
  • Large variations in formation stresses and unsystematically in-situ stresses measurements.
  • Large variations in the material properties of the formations and the limited amounts of material available for rock mechanics testing due to high-costed coring.
  • Acting forces on the formation around the wellbore such as mud chemistry, redistribution of stresses, temperature changes, etc.

Numerous wellbore stability models have been developed since the past decades in order to tackle wellbore instability problems and determine a safe mud window, however, these models have a number of shortcomings. Most of the published models have assumptions of an elastic rock material, material, a time-independent of borehole failure and no effect of the intermediate stress on the rock strength.

Recently, the models that consider the fully coupled poroelastic phenomenon require a lot of parameters, which may not available and time-consuming computation, such as the core data. Over the past decade, several contributions have been performed for the successful drilling of wells in the oil and gas industry. A wellbore stability analysis was carried out by Fuf et al.6 before drilling the first horizontal well in the German Sector of the North Sea region. Eight vertical offset wells data in the area were analyzed and used to develop a MEM in order to simulate the horizontal wellbore design and trajectory behavior prior execution.

Ong and Roegiers,7 suggested an anisotropic wellbore stability model in order to determine the stress around the well bore. The model led to deduce that the well bore collapse is affected by the degree of the rock strength in horizontal wellbore. They also found that pore pressure and Biot’s constant affect the shear failure, however, their effect is less obvious. Morita8 presented a borehole trajectory study effect on wellbore stability. The study deduced that an oriented wells have a non-uniform stress distribution around the bore hole.

Hodge et al.9 developed a time-dependent wellbore stability model by performing a fully coupled poroelastic model.  In this model, the stress changes around well bore induced by the fluid flow are taken in consideration using finite element method. In order to analyze the stability of the borehole, the developed model is utilized in various formation types, stress regimes, and drilling circumstances.

Rabaa et al.10 studied borehole instability for effective drilling and reservoir management determination. in order to minimize the risk of wellbore instabilities as wellbore breakouts for an extended reach horizontal hole, the study was used to identify the optimum mud weight and well azimuth.  They deduced that the horizontal wells in the direction of the maximum principal horizontal stress is preferable in order to maximize the margin of the wellbore stability and to minimize the minimum required mud weight during drilling.

Li and Purdy11 deduced two methods to estimate maximum horizontal stress. The first technique is based on the theory of equilibrium of three in-situ stresses components, the pore pressure, and the generalized Hooke’s law. In this technique, a decrease in the uncertainty of in-situ stress is achieved. The second one includes the drilling breakouts and induced near-wellbore stresses analyses using the Mohr-Coulomb failure criterion.

Qi et al.12 modeled the poroelasticity effect on wellbore stability for under balanced and overbalanced drilling conditions. An analytical coupled poroelastic modeling is studied for the over-balanced and underbalanced drilling scenarios. A time-dependent failure occurring inside the formation instead of at the wellbore wall is resulted.

Manshad et al.,13 performed a wellbore stability analysis for vertical, deviated and horizontal wells utilizing analytical and numerical techniques. In this stability analysis, various rock failure criteria such as Mohr-Coulomb, Modified Lade, Mogi–Coulomb, and Tresca yield criterion are used for the optimum well trajectory and mud weight determinations.  The predicted mud weight calculated using all these criteria is found giving reliable results.  Nevertheless, Tresca and Mohr-Coulomb criteria are found overestimating the minimum required mud pressure to maintain the wellbore stability. Additionally, another wellbore stability models used for horizontal and deviated wells based on in-situ stresses equations are presented by Halafawi14, Yi15, and Mohiuddin16. The role of rock strength criteria in wellbore stability and trajectory optimization is presented by Chabook17.

A good understanding of the preceded various chronological wellbore stability of the above models, their techniques and calculations is essential for selecting good practical instability prediction model for overcoming the resulting drilling instability wellbore problems. Additionally, since the rock is a porous medium, its mechanical response alters due to the fluid present inside the pores, and the limited data available, the poroelastic model with the same assumptions of previous authors will be assumed in order to take into account the phenomena of the interaction between the reservoir pressure and rock deformation, and to recommend a better practice for future operations.

Therefore, the main aim of this paper is to developed an integrated time-dependent well bore instability model in order to predict the wellbore stability issues in the pre-drilling stage and to simulate and analyze wells stability of RBS-91 field. Theory about borehole stability is presented for vertical and deviated wells with the different equations required for determining borehole fracturing and collapse. The developed model depends only on offset well-logs data and a less time-consuming mathematical descriptions so that the safest well path, as well as the optimum safe mud weight, can be determined. Additionally, the model is used to determine if this will as a candidate for underbalanced drilling or not.

Developed Wellbore Stability Model

To satisfy the objective of being able to run the developed model to predict wellbore instability problems anddetermine the optimum mud weight for future drilling activities, it is necessary to describe insitu stresses and pore pressure, circular wellbore stresses, cartesian stresses in three dimensions, rock failure criteria, rock mechanical properties and rock strength, and time-dependent wellbore stresses.

Insitu Stresses and Pore Pressure Prediction

The magnitude and orientation of in-situ stresses affect greatly the wellbore stability. The principal in-situ stresses are expressed as vertical stress ( σ v ) MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacaGGOaacceGae83Wdm3damaaBaaajuaibaWdbiaahAhaaKqb a+aabeaacaGGPaaaaa@3BD1@ , minimum horizontal stress ( σ h ) MathType@MTEF@5@5@+= feaagKart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacaGGOaGaeq4Wdm3damaaBaaajuaibaWdbiaadIgaaKqba+aa beaacaGGPaaaaa@3BB8@ and maximum horizontal stress ( σ H ) MathType@MTEF@5@5@+= feaagKart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacaGGOaGaeq4Wdm3damaaBaaajuaibaWdbiaadIeaaKqba+aa beaacaGGPaaaaa@3B98@ . In order to predict wellbore stability, these stresses are used to develop the geomechanical earth model (GEM). Several authors have presented various equations to determine thein-situ stresses using different assumptions and techniques as follows:

Vertical in-situ stress

The vertical stress or overburden stress is the main principle stress which direction is directing to the earth’s center. The magnitude of σv is estimated by the integration of rock densities at each incremental depth from surface to the depth of interest.15,18 At any depth, The rock has various lithology and porosity, therefore the rock density varies. Rock density data is most commonly acquired LWD data.
σ v = 0 H ρ b ( h )dh MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaaccmqcfaieaa aaaaaaa8qacqWFdpWCpaWaaSbaaKqbGeaapeGaaCODaaqcfa4daeqa a8qacqGH9aqpdaGfWbqabKqbG8aabaWdbiaaicdaa8aabaWdbiaahI eaaKqba+aabaWdbiabgUIiYdaacqWFbpGCpaWaaSbaaKqbGeaapeGa aCOyaaqcfa4daeqaa8qadaqadaWdaeaapeGaaCiAaaGaayjkaiaawM caaiaahsgacaWHObaaaa@48C5@ (1)

Minimum horizontal stress

In order to determine the minimum horizontal stress, the only fully reliable method is to fracture the formation and find the fracture closure pressure, this test known as Micro frac and Extended Leak-off (XLOT) tests.2 However, correlations and equations 2 through 6 shown in Table (1) also give a reasonable values.

Author/PublisherName

Min. Horizontal Stress Formula

Yi et al.15,Hudson et al.19, and Biot20

σ h = υ 1υ ( σ v α b P p )+ α b P p MathType@MTEF@5@5@+= feaagKart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacaqGdpWdamaaBaaajuaibaWdbiaabIgaaKqba+aabeaapeGa eyypa0ZaaSaaa8aabaWdbiaabw8aa8aabaWdbiaaigdacqGHsislca qGfpaaamaabmaapaqaa8qacaqGdpWdamaaBaaajuaibaWdbiaabAha aKqba+aabeaapeGaeyOeI0IaaeySd8aadaWgaaqcfasaa8qacaqGIb aajuaGpaqabaWdbiaabcfapaWaaSbaaKqbGeaapeGaaeiCaaqcfa4d aeqaaaWdbiaawIcacaGLPaaacqGHRaWkcaqGXoWdamaaBaaajuaiba WdbiaabkgaaKqba+aabeaapeGaaeiua8aadaWgaaqcfasaa8qacaqG Wbaapaqabaaaaa@51EB@ (2)

Ahmed et al.21, Cipolla et al.22, and Iverson23

σ h = υ 1υ ( σ v α b P p )+ α b P p + σ tec MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacaqGdpWdamaaBaaajuaibaWdbiaabIgaaKqba+aabeaapeGa eyypa0ZaaSaaa8aabaWdbiaabw8aa8aabaWdbiaaigdacqGHsislca qGfpaaamaabmaapaqaa8qacaqGdpWdamaaBaaajuaibaWdbiaabAha aKqba+aabeaapeGaeyOeI0IaaeySd8aadaWgaaqcfasaa8qacaqGIb aajuaGpaqabaWdbiaabcfapaWaaSbaaKqbGeaapeGaaeiCaaqcfa4d aeqaaaWdbiaawIcacaGLPaaacqGHRaWkcaqGXoWdamaaBaaajuaiba WdbiaabkgaaKqba+aabeaapeGaaeiua8aadaWgaaqcfasaa8qacaqG WbaajuaGpaqabaWdbiabgUcaRiabeo8aZ9aadaWgaaqcfasaa8qaca WG0bGaamyzaiaadogaaKqba+aabeaaaaa@5905@ (3)

Mike Mullen Equation19

σ h = σ v ( ν fast 1 ν fast )α P r ( 1 ν fast 1 ν fast ) MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacqaHdpWCpaWaaSbaaKqbGeaapeGaamiAaaqcfa4daeqaa8qa cqGH9aqpcqaHdpWCpaWaaSbaaKqbGeaapeGaamODaaqcfa4daeqaa8 qadaqadaWdaeaapeWaaSaaa8aabaWdbiabe27aU9aadaWgaaqcfasa a8qacaWGMbGaamyyaiaadohacaWG0baajuaGpaqabaaabaWdbiaaig dacqGHsislcqaH9oGBpaWaaSbaaKqbGeaapeGaamOzaiaadggacaWG ZbGaamiDaaqcfa4daeqaaaaaa8qacaGLOaGaayzkaaGaeyOeI0Iaeq ySdeMaamiua8aadaWgaaqcfasaa8qacaWGYbaajuaGpaqabaWdbmaa bmaapaqaa8qacaaIXaGaeyOeI0YaaSaaa8aabaWdbiabe27aU9aada Wgaaqcfasaa8qacaWGMbGaamyyaiaadohacaWG0baajuaGpaqabaaa baWdbiaaigdacqGHsislcqaH9oGBpaWaaSbaaKqbGeaapeGaamOzai aadggacaWGZbGaamiDaaqcfa4daeqaaaaaa8qacaGLOaGaayzkaaaa aa@67BC@ (4)

Blanton and Olson24

σ h =ν C 1 ε tec + C 2 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacqaHdpWCpaWaaSbaaKqbGeaapeGaamiAaaqcfa4daeqaa8qa cqGH9aqpcqaH9oGBcaWGdbWdamaaBaaajuaibaWdbiaaigdaaKqba+ aabeaapeGaeqyTdu2damaaBaaajuaibaWdbiaadshacaWGLbGaam4y aaqcfa4daeqaa8qacqGHRaWkcaWGdbWdamaaBaaajuaibaWdbiaaik daaKqba+aabeaaaaa@48CA@ (5)
Where
C 1 = E 1 ν 2 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacaWGdbWdamaaBaaajuaibaWdbiaaigdaaKqba+aabeaapeGa eyypa0ZaaSaaa8aabaWdbiaadweaa8aabaWdbiaaigdacqGHsislcq aH9oGBpaWaaWbaaeqajuaibaWdbiaaikdaaaaaaaaa@3FEC@
C 2 = ν σ V +( 12ν )α P p +E α t ΔT 1ν MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacaWGdbWdamaaBaaajuaibaWdbiaaikdaaKqba+aabeaapeGa eyypa0ZaaSaaa8aabaWdbiabe27aUjabeo8aZ9aadaWgaaqcfasaa8 qacaWGwbaajuaGpaqabaWdbiabgUcaRmaabmaapaqaa8qacaaIXaGa eyOeI0IaaGOmaiabe27aUbGaayjkaiaawMcaaiabeg7aHjaadcfapa WaaSbaaKqbGeaapeGaamiCaaqcfa4daeqaa8qacqGHRaWkcaWGfbGa aeiiaiabeg7aHjaabccacaWG0bGaaeiiaiabfs5aejaadsfaa8aaba WdbiaaigdacqGHsislcqaH9oGBaaaaaa@56FF@
ε tec = S h C ' 2 νC ' 1 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacqaH1oqzpaWaaSbaaKqbGeaapeGaamiDaiaadwgacaWGJbaa juaGpaqabaWdbiabg2da9maalaaapaqaa8qacaWGtbWdamaaBaaaju aibaWdbiaadIgaaKqba+aabeaapeGaeyOeI0Iaam4qaiaacEcapaWa aSbaaKqbGeaapeGaaGOmaaqcfa4daeqaaaqaa8qacqaH9oGBcaWGdb Gaai4ja8aadaWgaaqcfasaa8qacaaIXaaajuaGpaqabaaaaaaa@496F@

Harikrishnan and Hareland25

σ h = K o ( σ v α P p )+α P p MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacqaHdpWCpaWaaSbaaKqbGeaapeGaamiAaaqcfa4daeqaa8qa cqGH9aqpcaWGlbWdamaaBaaajuaibaWdbiaad+gaaKqba+aabeaape WaaeWaa8aabaWdbiabeo8aZ9aadaWgaaqcfasaa8qacaWG2baajuaG paqabaWdbiabgkHiTiabeg7aHjaadcfapaWaaSbaaKqbGeaapeGaam iCaaqcfa4daeqaaaWdbiaawIcacaGLPaaacqGHRaWkcqaHXoqycaWG qbWdamaaBaaajuaibaWdbiaadchaaKqba+aabeaaaaa@4E9D@ (6)
Where
K o =1sinβ MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacaWGlbWdamaaBaaajuaibaWdbiaad+gaaKqba+aabeaapeGa eyypa0JaaGymaiabgkHiTiaadohacaWGPbGaamOBaiabek7aIbaa@40AC@
β=arcsin( S 2 S 1 S 2 S 1 +4Δ ) MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacqaHYoGycqGH9aqpciGGHbGaaiOCaiaacogacaGGZbGaaiyA aiaac6gadaqadaWdaeaapeWaaSaaa8aabaWdbiaadofapaWaaSbaaK qbGeaapeGaaGOmaaqcfa4daeqaa8qacqGHsislcaWGtbWdamaaBaaa juaibaWdbiaaigdaaKqba+aabeaaaeaapeGaam4ua8aadaWgaaqcfa saa8qacaaIYaaajuaGpaqabaWdbiabgkHiTiaadofapaWaaSbaaKqb GeaapeGaaGymaaqcfa4daeqaa8qacqGHRaWkcaaI0aGaeuiLdqeaaa GaayjkaiaawMcaaaaa@5057@
S 1 = C o ( 1+ a s ( P e Δ ) ) b s MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacaWGtbWdamaaBaaajuaibaWdbiaaigdaaKqba+aabeaapeGa eyypa0Jaam4qa8aadaWgaaqcfasaa8qacaWGVbaajuaGpaqabaWdbm aabmaapaqaa8qacaaIXaGaey4kaSIaamyya8aadaWgaaqcfasaa8qa caWGZbaajuaGpaqabaWdbmaabmaapaqaa8qacaWGqbWdamaaBaaaju aibaWdbiaadwgaaKqba+aabeaapeGaeyOeI0IaaeiLdaGaayjkaiaa wMcaaaGaayjkaiaawMcaa8aadaahaaqabKqbGeaapeGaamOyaKqba+ aadaWgaaqcfasaa8qacaWGZbaapaqabaaaaaaa@4D50@
S 2 = C o ( 1+ a s ( P e +Δ ) ) b s MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacaWGtbWdamaaBaaajuaibaWdbiaaikdaaKqba+aabeaapeGa eyypa0Jaam4qa8aadaWgaaqcfasaa8qacaWGVbaajuaGpaqabaWdbm aabmaapaqaa8qacaaIXaGaey4kaSIaamyya8aadaWgaaqcfasaa8qa caWGZbaajuaGpaqabaWdbmaabmaapaqaa8qacaWGqbWdamaaBaaaju aibaWdbiaadwgaaKqba+aabeaapeGaey4kaSIaaeiLdaGaayjkaiaa wMcaaaGaayjkaiaawMcaa8aadaahaaqabKqbGeaapeGaamOyaKqba+ aadaWgaaqcfasaa8qacaWGZbaapaqabaaaaaaa@4D46@

Table 1 Minimum horizontal stress correlation and equations.

Maximum horizontal stress

Maximum horizontal stress magnitude and orientation can be determined from the inversion of calibration of borehole failure such as breakouts, washouts, drilling-induced fractures and drilling problems.15 However, several authors have presented various equations 7 through 10 which are appeared in Table (2) in order to a reasonable value for prediction modeling.

Author/Publisher Name

Max. Horizontal Stress Formula

Barton et al.26

σ H = C o +Δ P w +2 P r 12cos2θ σ h 1+2cos2θ 12cos θ MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacqaHdpWCpaWaaSbaaKqbGeaapeGaamisaaqcfa4daeqaa8qa cqGH9aqpdaWcaaWdaeaapeGaam4qa8aadaWgaaqcfasaa8qacaWGVb aajuaGpaqabaWdbiabgUcaRiaabs5acaWGqbWdamaaBaaajuaibaWd biaadEhaaKqba+aabeaapeGaey4kaSIaaGOmaiaadcfapaWaaSbaaK qbGeaapeGaamOCaaqcfa4daeqaaaqaa8qacaaIXaGaeyOeI0IaaGOm aiGacogacaGGVbGaai4CaiaaikdacqaH4oqCaaGaeyOeI0Iaeq4Wdm 3damaaBaaajuaibaWdbiaadIgaaKqba+aabeaapeWaaSaaa8aabaWd biaaigdacqGHRaWkcaaIYaGaci4yaiaac+gacaGGZbGaaGOmaiabeI 7aXbWdaeaapeGaaGymaiabgkHiTiaaikdacaWGJbGaam4Baiaadoha caqGGaGaeqiUdehaaaaa@63A7@ (7)

Mike Mullen Equation19

σ H = σ v ( ν slow 1 ν slow )α P r ( 1 ν slow 1 ν slow ) MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacqaHdpWCpaWaaSbaaKqbGeaapeGaamisaaqcfa4daeqaa8qa cqGH9aqpcqaHdpWCpaWaaSbaaKqbGeaapeGaamODaaqcfa4daeqaa8 qadaqadaWdaeaapeWaaSaaa8aabaWdbiabe27aU9aadaWgaaqcfasa a8qacaWGZbGaamiBaiaad+gacaWG3baajuaGpaqabaaabaWdbiaaig dacqGHsislcqaH9oGBpaWaaSbaaKqbGeaapeGaam4CaiaadYgacaWG VbGaam4Daaqcfa4daeqaaaaaa8qacaGLOaGaayzkaaGaeyOeI0Iaeq ySdeMaamiua8aadaWgaaqcfasaa8qacaWGYbaajuaGpaqabaWdbmaa bmaapaqaa8qacaaIXaGaeyOeI0YaaSaaa8aabaWdbiabe27aU9aada Wgaaqcfasaa8qacaWGZbGaamiBaiaad+gacaWG3baajuaGpaqabaaa baWdbiaaigdacqGHsislcqaH9oGBpaWaaSbaaKqbGeaapeGaam4Cai aadYgacaWGVbGaam4Daaqcfa4daeqaaaaaa8qacaGLOaGaayzkaaaa aa@67F8@ (8)

Addis et al.27,28

σ H σ h =ν( 1+ 1 K β )+ P p σ v [ 1ν( 1+ 1 K β ) ] MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qadaWcaaWdaeaapeGaae4Wd8aadaWgaaqcfasaa8qacaqGibaa juaGpaqabaaabaWdbiaabo8apaWaaSbaaKqbGeaapeGaaeiAaaqcfa 4daeqaaaaapeGaeyypa0JaaeyVdmaabmaapaqaa8qacaaIXaGaey4k aSYaaSaaa8aabaWdbiaaigdaa8aabaWdbiaabUeapaWaaSbaaKqbGe aapeGaaeOSdaqcfa4daeqaaaaaa8qacaGLOaGaayzkaaGaey4kaSYa aSaaa8aabaWdbiaabcfapaWaaSbaaKqbGeaapeGaaeiCaaqcfa4dae qaaaqaa8qacaqGdpWdamaaBaaajuaibaWdbiaabAhaaKqba+aabeaa aaWdbmaadmaapaqaa8qacaaIXaGaeyOeI0IaaeyVdmaabmaapaqaa8 qacaaIXaGaey4kaSYaaSaaa8aabaWdbiaaigdaa8aabaWdbiaabUea paWaaSbaaKqbGeaapeGaaeOSdaqcfa4daeqaaaaaa8qacaGLOaGaay zkaaaacaGLBbGaayzxaaaaaa@5AC4@ (9) for Normal Fault σ H σ h =ν( 1+ K β )+ P p σ v [ 1ν( 1+ K β ) ] MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qadaWcaaWdaeaapeGaae4Wd8aadaWgaaqcfasaa8qacaqGibaa juaGpaqabaaabaWdbiaabo8apaWaaSbaaKqbGeaapeGaaeiAaaqcfa 4daeqaaaaapeGaeyypa0JaaeyVdmaabmaapaqaa8qacaaIXaGaey4k aSIaae4sa8aadaWgaaqcfasaa8qacaqGYoaajuaGpaqabaaapeGaay jkaiaawMcaaiabgUcaRmaalaaapaqaa8qacaqGqbWdamaaBaaajuai baWdbiaabchaaKqba+aabeaaaeaapeGaae4Wd8aadaWgaaqcfasaa8 qacaqG2baajuaGpaqabaaaa8qadaWadaWdaeaapeGaaGymaiabgkHi Tiaab27adaqadaWdaeaapeGaaGymaiabgUcaRiaabUeapaWaaSbaaK qbGeaapeGaaeOSdaqcfa4daeqaaaWdbiaawIcacaGLPaaaaiaawUfa caGLDbaaaaa@58B2@ (10) for Thrust Fauly
Where
K β = sin(+2β)+sin sin( +2β )sin MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacaWGlbWdamaaBaaabaWdbiabek7aIbWdaeqaa8qacqGH9aqp daWcaaWdaeaapeGaci4CaiaacMgacaGGUbGaaiikaiabgwGiglabgU caRiaaikdacqaHYoGycaGGPaGaey4kaSIaci4CaiaacMgacaGGUbGa eyybIymapaqaa8qaciGGZbGaaiyAaiaac6gadaqadaWdaeaapeGaey ybIySaey4kaSIaaGOmaiabek7aIbGaayjkaiaawMcaaiabgkHiTiaa dohacaWGPbGaamOBaiabgwGigdaaaaa@575C@

Table 2 Maximum horizontal stress correlation and equations.

Pore Pressure Prediction

A formation pressure or pore pressure can be determined by kicks, resistivity logs, or sonic velocity logs but the most widely method to estimate the pore pressure is Eaton29 as follows:
P r = σ v ( σ v P rn ) ( Δ t norm Δ t log ) x MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacaWGqbWdamaaBaaajuaibaWdbiaadkhaaKqba+aabeaapeGa eyypa0Jaeq4Wdm3damaaBaaajuaibaWdbiaadAhaaKqba+aabeaape GaeyOeI0YaaeWaa8aabaWdbiabeo8aZ9aadaWgaaqcfasaa8qacaWG 2baajuaGpaqabaWdbiabgkHiTiaadcfapaWaaSbaaKqbGeaapeGaam OCaiaad6gaaKqba+aabeaaa8qacaGLOaGaayzkaaWaaeWaa8aabaWd bmaalaaapaqaaGGab8qacqWFuoarcaWG0bWdamaaBaaajuaibaWdbi aad6gacaWGVbGaamOCaiaad2gaaKqba+aabeaaaeaapeGae8hLdqKa amiDa8aadaWgaaqcfasaa8qaciGGSbGaai4BaiaacEgaaKqba+aabe aaaaaapeGaayjkaiaawMcaa8aadaahaaqabKqbGeaapeGaamiEaaaa aaa@5A76@ (11)

Circular Wellbore Stresses

Before making a borehole, a rock is loaded on all sides and has uniform stresses in all directions. This case is then defined as in situ stress state. When a borehole is drilled in the center of the formation region, the stress state around the hole will vary due to the new geometrical element. This state around the hole is described as a stress concentration. The two stress categories resulted due to conditions modifications are in-situ/rock stresses and stresses around the hole. The Kirsch equations2,3,30 and their derivatives are the most important equations related to applied rock mechanics. The Kirsch equations 2,3,30 are:

σ r = 1 2 ( σ x + σ y )( 1 R w 2 r 2 )+ 1 2 ( σ x σ y )( 1+3 R w 4 r 4 4 R w 2 r 2 )cos2θ+ τ xy ( 1+33 R w 4 r 4 4 R w 2 r 2 )sin2θ+ R w 2 r 2 MathType@MTEF@5@5@+= feaagKart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaacceqcfaieaa aaaaaaa8qacqWFdpWCpaWaaSbaaKqbGeaapeGaaCOCaaqcfa4daeqa a8qacqGH9aqpdaWcaaWdaeaapeGaaGymaaWdaeaapeGaaGOmaaaada qadaWdaeaapeGae83Wdm3damaaBaaajuaibaWdbiaahIhaaKqba+aa beaapeGaey4kaSIae83Wdm3damaaBaaajuaibaWdbiaahMhaaKqba+ aabeaaa8qacaGLOaGaayzkaaWaaeWaa8aabaWdbiaaigdacqGHsisl daWcaaWdaeaapeGaaCOua8aadaqhaaqcfasaa8qacaWH3baapaqaa8 qacaaIYaaaaaqcfa4daeaapeGaaCOCa8aadaahaaqabKqbGeaapeGa aGOmaaaaaaaajuaGcaGLOaGaayzkaaGaey4kaSYaaSaaa8aabaWdbi aaigdaa8aabaWdbiaaikdaaaWaaeWaa8aabaWdbiab=n8aZ9aadaWg aaqcfasaa8qacaWH4baajuaGpaqabaWdbiabgkHiTiab=n8aZ9aada Wgaaqcfasaa8qacaWH5baajuaGpaqabaaapeGaayjkaiaawMcaamaa bmaapaqaa8qacaaIXaGaey4kaSIaaG4mamaalaaapaqaa8qacaWHsb WdamaaDaaajuaibaWdbiaahEhaa8aabaWdbiaaisdaaaaajuaGpaqa a8qacaWHYbWdamaaCaaabeqcfasaa8qacaaI0aaaaaaajuaGcqGHsi slcaaI0aWaaSaaa8aabaWdbiaahkfapaWaa0baaKqbGeaapeGaaC4D aaWdaeaapeGaaGOmaaaaaKqba+aabaWdbiaahkhapaWaaWbaaeqaju aibaWdbiaaikdaaaaaaaqcfaOaayjkaiaawMcaaiGacogacaGGVbGa ai4CaiaaikdacqWF4oqCcqGHRaWkcqaHepaDpaWaaSbaaKqbGeaape GaaCiEaiaahMhaaKqba+aabeaapeWaaeWaa8aabaWdbiaaigdacqGH RaWkcaaIZaGaaG4mamaalaaapaqaa8qacaWHsbWdamaaDaaajuaiba WdbiaahEhaa8aabaWdbiaaisdaaaaajuaGpaqaa8qacaWHYbWdamaa Caaabeqcfasaa8qacaaI0aaaaaaajuaGcqGHsislcaaI0aWaaSaaa8 aabaWdbiaahkfapaWaa0baaKqbGeaapeGaaC4DaaWdaeaapeGaaGOm aaaaaKqba+aabaWdbiaahkhapaWaaWbaaeqajuaibaWdbiaaikdaaa aaaaqcfaOaayjkaiaawMcaaiGacohacaGGPbGaaiOBaiaaikdacqWF 4oqCcqGHRaWkdaWcaaWdaeaapeGaaCOua8aadaqhaaqcfasaa8qaca WH3baapaqaa8qacaaIYaaaaaqcfa4daeaapeGaaCOCa8aadaahaaqa bKqbGeaapeGaaGOmaaaaaaaaaa@9CC9@
σ θ = 1 2 ( σ x + σ y )( 1+ R w 2 r 2 )+ 1 2 ( σ x σ y )( 1+3 R w 4 r 4 )cos2θ+ τ xy ( 1+3 R w 4 r 4 )sin2θ+ R w 2 r 2 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaacceqcfaieaa aaaaaaa8qacqWFdpWCpaWaaSbaaKqbGeaapeGae8hUdehajuaGpaqa baWdbiabg2da9maalaaapaqaa8qacaaIXaaapaqaa8qacaaIYaaaam aabmaapaqaa8qacqWFdpWCpaWaaSbaaKqbGeaapeGaaCiEaaqcfa4d aeqaa8qacqGHRaWkcqWFdpWCpaWaaSbaaKqbGeaapeGaaCyEaaqcfa 4daeqaaaWdbiaawIcacaGLPaaadaqadaWdaeaapeGaaGymaiabgUca Rmaalaaapaqaa8qacaWHsbWdamaaDaaajuaibaWdbiaahEhaa8aaba WdbiaaikdaaaaajuaGpaqaa8qacaWHYbWdamaaCaaabeqcfasaa8qa caaIYaaaaaaaaKqbakaawIcacaGLPaaacqGHRaWkdaWcaaWdaeaape GaaGymaaWdaeaapeGaaGOmaaaadaqadaWdaeaapeGae83Wdm3damaa BaaajuaibaWdbiaahIhaaKqba+aabeaapeGaeyOeI0Iae83Wdm3dam aaBaaajuaibaWdbiaahMhaaKqba+aabeaaa8qacaGLOaGaayzkaaWa aeWaa8aabaWdbiaaigdacqGHRaWkcaaIZaWaaSaaa8aabaWdbiaahk fapaWaa0baaKqbGeaapeGaaC4DaaWdaeaapeGaaGinaaaaaKqba+aa baWdbiaahkhapaWaaWbaaeqajuaibaWdbiaaisdaaaaaaaqcfaOaay jkaiaawMcaaiGacogacaGGVbGaai4CaiaaikdaiiaacqGF4oqCcqGH RaWkcqaHepaDpaWaaSbaaKqbGeaapeGaaCiEaiaahMhaaKqba+aabe aapeWaaeWaa8aabaWdbiaaigdacqGHRaWkcaaIZaWaaSaaa8aabaWd biaahkfapaWaa0baaKqbGeaapeGaaC4DaaWdaeaapeGaaGinaaaaaK qba+aabaWdbiaahkhapaWaaWbaaeqajuaibaWdbiaaisdaaaaaaaqc faOaayjkaiaawMcaaiGacohacaGGPbGaaiOBaiaaikdacqGF4oqCcq GHRaWkdaWcaaWdaeaapeGaaCOua8aadaqhaaqcfasaa8qacaWH3baa paqaa8qacaaIYaaaaaqcfa4daeaapeGaaCOCa8aadaahaaqabKqbGe aapeGaaGOmaaaaaaaaaa@8C00@
σ z = σ zz 2ν( σ x σ y ) R w 2 r 2 cos2θ4ν τ xy R w 2 r 2 sin2θ MathType@MTEF@5@5@+= feaagKart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaaccaqcfaieaa aaaaaaa8qacqWFdpWCpaWaaSbaaKqbGeaapeGaaCOEaaqcfa4daeqa a8qacqGH9aqpcqWFdpWCpaWaaSbaaKqbGeaapeGaamOEaiaadQhaaK qba+aabeaapeGaeyOeI0IaaGOmaiabe27aUnaabmaapaqaa8qacqWF dpWCpaWaaSbaaKqbGeaapeGaaCiEaaqcfa4daeqaa8qacqGHsislcq WFdpWCpaWaaSbaaKqbGeaapeGaaCyEaaqcfa4daeqaaaWdbiaawIca caGLPaaadaWcaaWdaeaapeGaaCOua8aadaqhaaqcfasaa8qacaWH3b aapaqaa8qacaaIYaaaaaqcfa4daeaapeGaaCOCa8aadaahaaqabKqb GeaapeGaaGOmaaaaaaqcfaOaci4yaiaac+gacaGGZbGaaGOmaiab=H 7aXjabgkHiTiaaisdaiiqacqGF9oGBcqGFepaDpaWaaSbaaKqbGeaa peGaaCiEaiaahMhaaKqba+aabeaapeWaaSaaa8aabaWdbiaahkfapa Waa0baaKqbGeaapeGaaC4DaaWdaeaapeGaaGOmaaaaaKqba+aabaWd biaahkhapaWaaWbaaeqajuaibaWdbiaaikdaaaaaaKqbakGacohaca GGPbGaaiOBaiaaikdacqWF4oqCaaa@6E46@
τ rθ ={ 1 2 ( σ x σ y )sin2θ+ τ xy cos2θ }( 13 R w 4 r 4 +2 R w 2 r 2 ) MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacqaHepaDpaWaaSbaaKqbGeaapeGaaCOCaGGaaiab=H7aXbqc fa4daeqaa8qacqGH9aqpdaGadaWdaeaapeWaaSaaa8aabaWdbiaaig daa8aabaWdbiaaikdaaaWaaeWaa8aabaWdbiab=n8aZ9aadaWgaaqc fasaa8qacaWH4baajuaGpaqabaWdbiabgkHiTiab=n8aZ9aadaWgaa qcfasaa8qacaWH5baajuaGpaqabaaapeGaayjkaiaawMcaaiGacoha caGGPbGaaiOBaiaaikdacqWF4oqCcqGHRaWkcqaHepaDpaWaaSbaaK qbGeaapeGaaCiEaiaahMhaaKqba+aabeaapeGaci4yaiaac+gacaGG ZbGaaGOmaiab=H7aXbGaay5Eaiaaw2haamaabmaapaqaa8qacaaIXa GaeyOeI0IaaG4mamaalaaapaqaa8qacaWHsbWdamaaDaaajuaibaWd biaahEhaa8aabaWdbiaaisdaaaaajuaGpaqaa8qacaWHYbWdamaaCa aabeqcfasaa8qacaaI0aaaaaaajuaGcqGHRaWkcaaIYaWaaSaaa8aa baWdbiaahkfapaWaa0baaKqbGeaapeGaaC4DaaWdaeaapeGaaGOmaa aaaKqba+aabaWdbiaahkhapaWaaWbaaeqajuaibaWdbiaaikdaaaaa aaqcfaOaayjkaiaawMcaaaaa@6F03@
τ rz ={ τ xz cosθ+ τ yz sinθ }( 1 R w 2 r 2 ) MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaacceqcfaieaa aaaaaaa8qacqWFepaDpaWaaSbaaKqbGeaapeGaaCOCaiaahQhaaKqb a+aabeaapeGaeyypa0ZaaiWaa8aabaWdbiab=r8a09aadaWgaaqcfa saa8qacaWG4bGaamOEaaqcfa4daeqaa8qacaWHJbGaaC4Baiaahoha cqWF4oqCcqGHRaWkcqWFepaDpaWaaSbaaKqbGeaapeGaaCyEaiaahQ haaKqba+aabeaapeGaaC4CaiaahMgacaWHUbGae8hUdehacaGL7bGa ayzFaaWaaeWaa8aabaWdbiaaigdacqGHsisldaWcaaWdaeaapeGaaC Oua8aadaqhaaqcfasaa8qacaWH3baapaqaa8qacaaIYaaaaaqcfa4d aeaapeGaaCOCa8aadaahaaqabKqbGeaapeGaaGOmaaaaaaaajuaGca GLOaGaayzkaaaaaa@5CA4@
τ rz ={ τ xz cosθ+ τ yz sinθ }( 1+ R w 2 r 2 ) MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaacceqcfaieaa aaaaaaa8qacqWFepaDpaWaaSbaaKqbGeaapeGaaCOCaiaahQhaaKqb a+aabeaapeGaeyypa0ZaaiWaa8aabaWdbiabgkHiTiab=r8a09aada Wgaaqcfasaa8qacaWG4bGaamOEaaqcfa4daeqaa8qacaWHJbGaaC4B aiaahohacqWF4oqCcqGHRaWkcqWFepaDpaWaaSbaaKqbGeaapeGaaC yEaiaahQhaaKqba+aabeaapeGaaC4CaiaahMgacaWHUbGae8hUdeha caGL7bGaayzFaaWaaeWaa8aabaWdbiaaigdacqGHRaWkdaWcaaWdae aapeGaaCOua8aadaqhaaqcfasaa8qacaWH3baapaqaa8qacaaIYaaa aaqcfa4daeaapeGaaCOCa8aadaahaaqabKqbGeaapeGaaGOmaaaaaa aajuaGcaGLOaGaayzkaaaaaa@5D86@ (12)

Now there is an expression for the borehole wall or the stress state in the adjacent formation. At the borehole wall (r=a), the equations are reduced to:
Radial stress: σ r = P w MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaacceqcfaieaa aaaaaaa8qacqWFdpWCpaWaaSbaaKqbGeaapeGaamOCaaqcfa4daeqa a8qacqGH9aqpcaWGqbWdamaaBaaajuaibaWdbiaadEhaaKqba+aabe aaaaa@3E62@ (13)

Tangential stress:
σ θ = σ x + σ y + P w 2γ( σ x σ y )cos( 2θ )4 τ xy sin( 2θ ) MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaacceqcfaieaa aaaaaaa8qacqWFdpWCpaWaaSbaaKqbGeaapeGae8hUdehajuaGpaqa baWdbiabg2da9iab=n8aZ9aadaWgaaqcfasaa8qacaWH4baajuaGpa qabaWdbiabgUcaRiab=n8aZ9aadaWgaaqcfasaa8qacaWH5baajuaG paqabaWdbiabgUcaRiaahcfapaWaaSbaaKqbGeaapeGaaC4Daaqcfa 4daeqaa8qacqGHsislcaaIYaGae83SdC2aaeWaa8aabaWdbiab=n8a Z9aadaWgaaqcfasaa8qacaWH4baajuaGpaqabaWdbiabgkHiTiab=n 8aZ9aadaWgaaqcfasaa8qacaWH5baajuaGpaqabaaapeGaayjkaiaa wMcaaiGacogacaGGVbGaai4Camaabmaapaqaa8qacaaIYaGae8hUde hacaGLOaGaayzkaaGaeyOeI0IaaGinaiab=r8a09aadaWgaaqcfasa a8qacaWH4bGaaCyEaaqcfa4daeqaa8qaciGGZbGaaiyAaiaac6gada qadaWdaeaapeGaaGOmaiab=H7aXbGaayjkaiaawMcaaaaa@6AA0@

Axial stress, plane strain:

σ z = σ zz 2γ( σ x σ y )cos( 2θ )4μ τ xy sin( 2θ ) MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaacceqcfaieaa aaaaaaa8qacqWFdpWCpaWaaSbaaKqbGeaapeGaaCOEaaqcfa4daeqa a8qacqGH9aqpcqWFdpWCpaWaaSbaaKqbGeaapeGaaCOEaiaahQhaaK qba+aabeaapeGaeyOeI0IaaGOmaiab=n7aNnaabmaapaqaa8qacqWF dpWCpaWaaSbaaKqbGeaapeGaaCiEaaqcfa4daeqaa8qacqGHsislcq WFdpWCpaWaaSbaaKqbGeaapeGaaCyEaaqcfa4daeqaaaWdbiaawIca caGLPaaaciGGJbGaai4BaiaacohadaqadaWdaeaapeGaaGOmaiab=H 7aXbGaayjkaiaawMcaaiabgkHiTiaaisdaiiaacqGF8oqBcqWFepaD paWaaSbaaKqbGeaapeGaaCiEaiaahMhaaKqba+aabeaapeGaci4Cai aacMgacaGGUbWaaeWaa8aabaWdbiaaikdacqWF4oqCaiaawIcacaGL Paaaaaa@641E@
Axial stress, plane stress: σ z = σ zz MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaacceqcfaieaa aaaaaaa8qacqWFdpWCpaWaaSbaaKqbGeaapeGaaCOEaaqcfa4daeqa a8qacqGH9aqpcqWFdpWCpaWaaSbaaKqbGeaapeGaaCOEaiaahQhaa8 aabeaaaaa@3FD3@
Shear stress:, σ θz =2( τ yz cosθ τ yz sinθ ) MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaacceqcfaieaa aaaaaaa8qacqWFdpWCpaWaaSbaaKqbGeaapeGae8hUdeNaaCOEaaqc fa4daeqaa8qacqGH9aqpcaaIYaWaaeWaa8aabaWdbiab=r8a09aada Wgaaqcfasaa8qacaWH5bGaaCOEaaqcfa4daeqaa8qacaWHJbGaaC4B aiaahohacqWF4oqCcqGHsislcqWFepaDpaWaaSbaaKqbGeaapeGaaC yEaiaahQhaaKqba+aabeaapeGaaC4CaiaahMgacaWHUbGae8hUdeha caGLOaGaayzkaaaaaa@537B@ τ rz = τ rθ MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaacceqcfaieaa aaaaaaa8qacqWFepaDpaWaaSbaaKqbGeaapeGaaCOCaiaahQhaaKqb a+aabeaapeGaeyypa0Jae8hXdq3damaaBaaajuaibaWdbiaahkhacq WF4oqCaKqba+aabeaaaaa@4206@

Cartesian Stresses in three dimensions

In the petroleum industry, three principle in-situ stresses are known: the vertical or overburden stress (sv), and the maximum and minimum horizontal stresses (sH and sh). Since the Kirsch equations 2,3,30 supposes the horizontal, vertical, and the borehole orientation may be in any direction, these stresses should consequently be transformed into Cartesian system x, y, and z and represented as stresses sx, sy and sz. Equations 14 represent all transformed stress components:

σ x =( σ H cos 2 φ+ σ h sin 2 φ ) cos 2 γ+ σ v sin 2 γ MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacqaHdpWCpaWaaSbaaKqbGeaapeGaamiEaaqcfa4daeqaa8qa cqGH9aqpdaqadaWdaeaapeGaeq4Wdm3damaaBaaajuaibaWdbiaadI eaaKqba+aabeaapeGaci4yaiaac+gacaGGZbWdamaaCaaabeqcfasa a8qacaaIYaaaaKqbakabeA8aQjabgUcaRiabeo8aZ9aadaWgaaqcfa saa8qacaWGObaajuaGpaqabaWdbiGacohacaGGPbGaaiOBa8aadaah aaqabKqbGeaapeGaaGOmaaaajuaGcqaHgpGAaiaawIcacaGLPaaaci GGJbGaai4BaiaacohapaWaaWbaaeqajuaibaWdbiaaikdaaaqcfaOa eq4SdCMaey4kaSIaeq4Wdm3damaaBaaajuaibaWdbiaadAhaaKqba+ aabeaapeGaci4CaiaacMgacaGGUbWdamaaCaaabeqcfasaa8qacaaI YaaaaKqbakabeo7aNbaa@6343@

σ y =( σ H sin 2 φ+ σ h cos 2 φ ) MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacqaHdpWCpaWaaSbaaKqbGeaapeGaamyEaaqcfa4daeqaa8qa cqGH9aqpdaqadaWdaeaapeGaeq4Wdm3damaaBaaajuaibaWdbiaadI eaaKqba+aabeaapeGaci4CaiaacMgacaGGUbWdamaaCaaabeqcfasa a8qacaaIYaaaaKqbakabeA8aQjabgUcaRiabeo8aZ9aadaWgaaqcfa saa8qacaWGObaajuaGpaqabaWdbiGacogacaGGVbGaai4Ca8aadaah aaqabKqbGeaapeGaaGOmaaaajuaGcqaHgpGAaiaawIcacaGLPaaaaa a@521E@

σ zz =( σ H cos 2 φ+ σ h sin 2 φ ) sin 2 γ+ σ v cos 2 γ MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacqaHdpWCpaWaaSbaaKqbGeaapeGaamOEaiaadQhaaKqba+aa beaapeGaeyypa0ZaaeWaa8aabaWdbiabeo8aZ9aadaWgaaqcfasaa8 qacaWGibaajuaGpaqabaWdbiGacogacaGGVbGaai4Ca8aadaahaaqa bKqbGeaapeGaaGOmaaaajuaGcqaHgpGAcqGHRaWkcqaHdpWCpaWaaS baaKqbGeaapeGaamiAaaqcfa4daeqaa8qaciGGZbGaaiyAaiaac6ga paWaaWbaaeqajuaibaWdbiaaikdaaaqcfaOaeqOXdOgacaGLOaGaay zkaaGaci4CaiaacMgacaGGUbWdamaaCaaabeqcfasaa8qacaaIYaaa aKqbakabeo7aNjabgUcaRiabeo8aZ9aadaWgaaqcfasaa8qacaWG2b aajuaGpaqabaWdbiGacogacaGGVbGaai4Ca8aadaahaaqabKqbGeaa peGaaGOmaaaajuaGcqaHZoWzaaa@6444@

τ yz = 1 2 ( σ h σ H )sinsin( 2φ )sinγ MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacqaHepaDpaWaaSbaaKqbGeaapeGaamyEaiaadQhaaKqba+aa beaapeGaeyypa0ZaaSaaa8aabaWdbiaaigdaa8aabaWdbiaaikdaaa WaaeWaa8aabaWdbiabeo8aZ9aadaWgaaqcfasaa8qacaWGObaajuaG paqabaWdbiabgkHiTiabeo8aZ9aadaWgaaqcfasaa8qacaWGibaaju aGpaqabaaapeGaayjkaiaawMcaaiGacohacaGGPbGaaiOBaiGacoha caGGPbGaaiOBamaabmaapaqaa8qacaaIYaGaeqOXdOgacaGLOaGaay zkaaGaci4CaiaacMgacaGGUbGaeq4SdCgaaa@56A8@

τ xz = 1 2 ( σ H cos 2 φ+ σ h sin 2 φ σ v )sin( 2γ ) MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacqaHepaDpaWaaSbaaKqbGeaapeGaamiEaiaadQhaaKqba+aa beaapeGaeyypa0ZaaSaaa8aabaWdbiaaigdaa8aabaWdbiaaikdaaa WaaeWaa8aabaWdbiabeo8aZ9aadaWgaaqcfasaa8qacaWGibaajuaG paqabaWdbiGacogacaGGVbGaai4Ca8aadaahaaqabKqbGeaapeGaaG OmaaaajuaGcqaHgpGAcqGHRaWkcqaHdpWCpaWaaSbaaKqbGeaapeGa amiAaaqcfa4daeqaa8qaciGGZbGaaiyAaiaac6gapaWaaWbaaeqaju aibaWdbiaaikdaaaqcfaOaeqOXdOMaeyOeI0Iaeq4Wdm3damaaBaaa juaibaWdbiaadAhaaKqba+aabeaaa8qacaGLOaGaayzkaaGaci4Cai aacMgacaGGUbWaaeWaa8aabaWdbiaaikdacqaHZoWzaiaawIcacaGL Paaaaaa@608C@

τ xy = 1 2 ( σ h σ H )sin( 2φ )cosγ MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacqaHepaDpaWaaSbaaKqbGeaapeGaamiEaiaadMhaaKqba+aa beaapeGaeyypa0ZaaSaaa8aabaWdbiaaigdaa8aabaWdbiaaikdaaa WaaeWaa8aabaWdbiabeo8aZ9aadaWgaaqcfasaa8qacaWGObaajuaG paqabaWdbiabgkHiTiabeo8aZ9aadaWgaaqcfasaa8qacaWGibaaju aGpaqabaaapeGaayjkaiaawMcaaiGacohacaGGPbGaaiOBamaabmaa paqaa8qacaaIYaGaeqOXdOgacaGLOaGaayzkaaGaci4yaiaac+gaca GGZbGaeq4SdCgaaa@53C9@ (14)

All equations required to analyze failusres of boreholes are now defined.

Rock Failure Criteria

Formation failure criteria identify, clearly and definitely, stress conditions at failure. Common formation failure criteria as shown in Table (3) can be classified based on two main characteristics (linear or nonlinear form, and considering the effect of intermediate principal stress on the rock strength). More details and discussion are presented by Rahimi31 and Halafawi.32

Failure Criterion Name

Failure Criterion Formula

Mohr-Coulomb

τ=μσ+C MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacaqGepGaeyypa0JaaeiVdiaabo8acqGHRaWkcaqGdbaaaa@3D28@ , μ=tan MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacaqG8oGaeyypa0JaaeiDaiaabggacaqGUbGaeqybIymaaa@3D30@

Mogi-Coulomb

τ oct =a+ m,2 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacaqGepWdamaaBaaajuaibaWdbiaab+gacaqGJbGaaeiDaaqc fa4daeqaa8qacqGH9aqpcaqGHbGaey4kaSIaaeOyaiaabo8apaWaaS baaKqbGeaapeGaaeyBaiaacYcacaaIYaaajuaGpaqabaaaaa@443A@
σ m,2 = 1 3 ( σ 1 + σ 3 ) MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacaqGdpWdamaaBaaajuaibaWdbiaab2gacaGGSaGaaGOmaaqc fa4daeqaa8qacqGH9aqpdaWcaaWdaeaapeGaaGymaaWdaeaapeGaaG 4maaaadaqadaWdaeaapeGaae4Wd8aadaWgaaqcfasaa8qacaaIXaaa juaGpaqabaWdbiabgUcaRiaabo8apaWaaSbaaKqbGeaapeGaaG4maa qcfa4daeqaaaWdbiaawIcacaGLPaaaaaa@46FB@
τ oct = 1 3 ( σ 1 σ 2 ) 2 + ( σ 1 σ 3 ) 2 + ( σ 2 σ 3 ) 2 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacaqGepWdamaaBaaajuaibaWdbiaab+gacaqGJbGaaeiDaaqc fa4daeqaa8qacqGH9aqpdaWcaaWdaeaapeGaaGymaaWdaeaapeGaaG 4maaaadaGcaaWdaeaapeWaaeWaa8aabaWdbiaabo8apaWaaSbaaKqb GeaapeGaaGymaaqcfa4daeqaa8qacqGHsislcaqGdpWdamaaBaaaju aibaWdbiaaikdaaKqba+aabeaaa8qacaGLOaGaayzkaaWdamaaCaaa beqcfasaa8qacaaIYaaaaKqbakabgUcaRmaabmaapaqaa8qacaqGdp WdamaaBaaajuaibaWdbiaaigdaaKqba+aabeaapeGaeyOeI0Iaae4W d8aadaWgaaqcfasaa8qacaaIZaaajuaGpaqabaaapeGaayjkaiaawM caa8aadaahaaqabKqbGeaapeGaaGOmaaaajuaGcqGHRaWkdaqadaWd aeaapeGaae4Wd8aadaWgaaqcfasaa8qacaaIYaaajuaGpaqabaWdbi abgkHiTiaabo8apaWaaSbaaKqbGeaapeGaaG4maaqcfa4daeqaaaWd biaawIcacaGLPaaapaWaaWbaaeqajuaibaWdbiaaikdaaaaajuaGbe aaaaa@6042@
a= 2 2 3 C 0 q+1 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacaqGHbGaeyypa0ZaaSaaa8aabaWdbiaaikdadaGcaaWdaeaa peGaaGOmaaqabaaapaqaa8qacaaIZaaaamaalaaapaqaa8qacaqGdb WdamaaBaaajuaibaWdbiaaicdaaKqba+aabeaaaeaapeGaaeyCaiab gUcaRiaaigdaaaaaaa@409C@ b= 2 2 3 q1 q+1 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacaqGIbGaeyypa0ZaaSaaa8aabaWdbiaaikdadaGcaaWdaeaa peGaaGOmaaqabaaapaqaa8qacaaIZaaaamaalaaapaqaa8qacaqGXb GaeyOeI0IaaGymaaWdaeaapeGaaeyCaiabgUcaRiaaigdaaaaaaa@40BD@

Tresca

( σ 1 + σ 3 ) 2 =C= τ max MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qadaWcaaWdaeaapeWaaeWaa8aabaWdbiaabo8apaWaaSbaaKqb GeaapeGaaGymaaqcfa4daeqaa8qacqGHRaWkcaqGdpWdamaaBaaaju aibaWdbiaaiodaaKqba+aabeaaa8qacaGLOaGaayzkaaaapaqaa8qa caaIYaaaaiabg2da9iaaboeacqGH9aqpcaqGepWdamaaBaaajuaiba WdbiGac2gacaGGHbGaaiiEaaqcfa4daeqaaaaa@4874@ , C O 2 =C MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qadaWcaaWdaeaapeGaae4qa8aadaWgaaqcfasaa8qacaqGpbaa juaGpaqabaaabaWdbiaaikdaaaGaeyypa0Jaae4qaaaa@3C0F@

Von Mises

J 2 = ( σ 1 σ 2 ) 2 + ( σ 1 σ 3 ) 2 + ( σ 2 σ 3 ) 2 6 = C O 3 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qadaGcaaWdaeaapeGaaeOsa8aadaWgaaqcfasaa8qacaaIYaaa juaGpaqabaaapeqabaGaeyypa0ZaaOaaa8aabaWdbmaalaaapaqaa8 qadaqadaWdaeaapeGaae4Wd8aadaWgaaqcfasaa8qacaaIXaaajuaG paqabaWdbiabgkHiTiaabo8apaWaaSbaaKqbGeaapeGaaGOmaaqcfa 4daeqaaaWdbiaawIcacaGLPaaapaWaaWbaaKqbGeqabaWdbiaaikda aaqcfaOaey4kaSYaaeWaa8aabaWdbiaabo8apaWaaSbaaKqbGeaape GaaGymaaqcfa4daeqaa8qacqGHsislcaqGdpWdamaaBaaajuaibaWd biaaiodaaKqba+aabeaaa8qacaGLOaGaayzkaaWdamaaCaaabeqcfa saa8qacaaIYaaaaKqbakabgUcaRmaabmaapaqaa8qacaqGdpWdamaa BaaajuaibaWdbiaaikdaaKqba+aabeaapeGaeyOeI0Iaae4Wd8aada Wgaaqcfasaa8qacaaIZaaajuaGpaqabaaapeGaayjkaiaawMcaa8aa daahaaqabKqbGeaapeGaaGOmaaaaaKqba+aabaWdbiaaiAdaaaaabe aacqGH9aqpdaWcaaWdaeaapeGaae4qa8aadaWgaaqcfasaa8qacaqG pbaajuaGpaqabaaabaWdbiaaiodaaaaaaa@61CE@

Drucker-Prager

J 2 =k+ αJ 1 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qadaGcaaWdaeaapeGaaeOsa8aadaWgaaqcfasaa8qacaaIYaaa juaGpaqabaaapeqabaGaeyypa0Jaae4AaiabgUcaRiaabg7acaqGkb WdamaaBaaajuaibaWdbiaaigdaaKqba+aabeaaaaa@4018@ , J 1 = σ 1 + σ 2 + σ 3 3 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacaqGkbWdamaaBaaajuaibaWdbiaaigdaaKqba+aabeaapeGa eyypa0ZaaSaaa8aabaWdbiaabo8apaWaaSbaaKqbGeaapeGaaGymaa qcfa4daeqaa8qacqGHRaWkcaqGdpWdamaaBaaajuaibaWdbiaaikda aKqba+aabeaapeGaey4kaSIaae4Wd8aadaWgaaqcfasaa8qacaaIZa aajuaGpaqabaaabaWdbiaaiodaaaaaaa@465E@

Hoek-Brown

σ 1 = σ 3 + mC 0 σ 3 + sC O 2 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacaqGdpWdamaaBaaajuaibaWdbiaaigdaaKqba+aabeaapeGa eyypa0Jaae4Wd8aadaWgaaqcfasaa8qacaaIZaaajuaGpaqabaWdbi abgUcaRmaakaaapaqaa8qacaqGTbGaae4qa8aadaWgaaqcfasaa8qa caaIWaaajuaGpaqabaWdbiaabo8apaWaaSbaaKqbGeaapeGaaG4maa qcfa4daeqaa8qacqGHRaWkcaqGZbGaae4qa8aadaqhaaqcfasaa8qa caqGpbaapaqaa8qacaaIYaaaaaqcfayabaaaaa@4AF0@

Modified Lade

I '' 1 3 I '' 3 = η 1 +27 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qadaWcaaWdaeaapeGaaeysa8aadaahaaqabeaapeGaae4jaiaa bEcaaaWdamaaDaaajuaibaWdbiaaigdaa8aabaWdbiaaiodaaaaaju aGpaqaa8qacaqGjbWdamaaCaaabeqaa8qacaqGNaGaae4jaaaapaWa aSbaaKqbGeaapeGaaG4maaqcfa4daeqaaaaapeGaeyypa0Jaae4Td8 aadaWgaaqcfasaa8qacaaIXaaajuaGpaqabaWdbiabgUcaRiaaikda caaI3aaaaa@4699@
I'' 1 =( σ 1 +S )+( σ 2 +S )+( σ 3 +S ) MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacaqGjbGaae4jaiaabEcapaWaaSbaaKqbGeaapeGaaGymaaqc fa4daeqaa8qacqGH9aqpdaqadaWdaeaapeGaae4Wd8aadaWgaaqcfa saa8qacaaIXaaajuaGpaqabaWdbiabgUcaRiaabofaaiaawIcacaGL PaaacqGHRaWkdaqadaWdaeaapeGaae4Wd8aadaWgaaqcfasaa8qaca aIYaaajuaGpaqabaWdbiabgUcaRiaabofaaiaawIcacaGLPaaacqGH RaWkdaqadaWdaeaapeGaae4Wd8aadaWgaaqcfasaa8qacaaIZaaaju aGpaqabaWdbiabgUcaRiaabofaaiaawIcacaGLPaaaaaa@50E5@
I'' 3 =( σ 1 +S ).( σ 2 +S ).( σ 3 +S ) MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacaqGjbGaae4jaiaabEcapaWaaSbaaKqbGeaapeGaaG4maaqc fa4daeqaa8qacqGH9aqpdaqadaWdaeaapeGaae4Wd8aadaWgaaqcfa saa8qacaaIXaaajuaGpaqabaWdbiabgUcaRiaabofaaiaawIcacaGL PaaacaqGUaWaaeWaa8aabaWdbiaabo8apaWaaSbaaKqbGeaapeGaaG Omaaqcfa4daeqaa8qacqGHRaWkcaqGtbaacaGLOaGaayzkaaGaaeOl amaabmaapaqaa8qacaqGdpWdamaaBaaajuaibaWdbiaaiodaaKqba+ aabeaapeGaey4kaSIaae4uaaGaayjkaiaawMcaaaaa@5085@

Modified Wiebols-Cook

J 2 =A+ BJ 1 + CJ 1 2 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qadaGcaaWdaeaapeGaaeOsa8aadaWgaaqcfasaa8qacaaIYaaa juaGpaqabaaapeqabaGaeyypa0JaaeyqaiabgUcaRiaabkeacaqGkb WdamaaBaaajuaibaWdbiaaigdaaKqba+aabeaapeGaey4kaSIaae4q aiaabQeapaWaaSbaaKqbGeaapeGaaGymaaqcfa4daeqaamaaCaaaju aibeqaa8qacaaIYaaaaaaa@44E3@

Griffith

( σ 1 σ 3 ) 2 =8 T O ( σ 1 + σ 3 ) MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qadaqadaWdaeaapeGaae4Wd8aadaWgaaqcfasaa8qacaaIXaaa juaGpaqabaWdbiabgkHiTiaabo8apaWaaSbaaKqbGeaapeGaaG4maa qcfa4daeqaaaWdbiaawIcacaGLPaaapaWaaWbaaeqajuaibaWdbiaa ikdaaaqcfaOaeyypa0JaaGioaiaabsfapaWaaSbaaKqbGeaapeGaae 4taaqcfa4daeqaa8qadaqadaWdaeaapeGaae4Wd8aadaWgaaqcfasa a8qacaaIXaaajuaGpaqabaWdbiabgUcaRiaabo8apaWaaSbaaKqbGe aapeGaaG4maaqcfa4daeqaaaWdbiaawIcacaGLPaaaaaa@4E89@
σ 3 = T O IF( σ 1 +3 σ 3 )<0,and T O = C O 8 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacaqGdpWdamaaBaaajuaibaWdbiaaiodaaKqba+aabeaapeGa eyypa0JaeyOeI0Iaaeiva8aadaWgaaqcfasaa8qacaqGpbaajuaGpa qabaWdbiaabMeacaqGgbWaaeWaa8aabaWdbiaabo8apaWaaSbaaKqb GeaapeGaaGymaaqcfa4daeqaa8qacqGHRaWkcaaIZaGaae4Wd8aada Wgaaqcfasaa8qacaaIZaaajuaGpaqabaaapeGaayjkaiaawMcaaiab gYda8iaaicdacaGGSaGaamyyaiaad6gacaWGKbGaaeiva8aadaWgaa qcfasaa8qacaqGpbaajuaGpaqabaWdbiabg2da9maalaaapaqaa8qa caqGdbWdamaaBaaajuaibaWdbiaab+eaaKqba+aabeaaaeaapeGaaG ioaaaaaaa@5637@

Modified Griffith

σ 1 [ μ 2 +1 μ ] σ 3 [ μ 2 +1 +μ ]=4 T O MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacqaHdpWCpaWaaSbaaKqbGeaapeGaaGymaaqcfa4daeqaa8qa daWadaWdaeaapeWaaOaaa8aabaWdbiabeY7aT9aadaahaaqabKqbGe aapeGaaGOmaaaajuaGcqGHRaWkcaaIXaaabeaacqGHsislcqaH8oqB aiaawUfacaGLDbaacqGHsislcqaHdpWCpaWaaSbaaKqbGeaapeGaaG 4maaqcfa4daeqaa8qadaWadaWdaeaapeWaaOaaa8aabaWdbiabeY7a T9aadaahaaqabKqbGeaapeGaaGOmaaaajuaGcqGHRaWkcaaIXaaabe aacqGHRaWkcqaH8oqBaiaawUfacaGLDbaacqGH9aqpcaaI0aGaamiv a8aadaWgaaqcfasaa8qacaWGpbaajuaGpaqabaaaaa@5715@
4 T O = 4 μ 2 +1 μ MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacaaI0aGaamiva8aadaWgaaqcfasaa8qacaWGpbaajuaGpaqa baWdbiabg2da9maalaaapaqaa8qacaaI0aaapaqaa8qadaGcaaWdae aapeGaeqiVd02damaaCaaabeqcfasaa8qacaaIYaaaaKqbakabgUca RiaaigdaaeqaaiabgkHiTiabeY7aTbaaaaa@441B@

Murrel

( σ 1 σ 3 ) 2 + ( σ 1 σ 2 ) 2 + ( σ 2 σ 3 ) 2 =24 T O ( σ 1 + σ 2 + σ 3 ) MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qadaqadaWdaeaapeGaeq4Wdm3damaaBaaajuaibaWdbiaaigda aKqba+aabeaapeGaeyOeI0Iaeq4Wdm3damaaBaaajuaibaWdbiaaio daaKqba+aabeaaa8qacaGLOaGaayzkaaWdamaaCaaabeqcfasaa8qa caaIYaaaaKqbakabgUcaRmaabmaapaqaa8qacqaHdpWCpaWaaSbaaK qbGeaapeGaaGymaaqcfa4daeqaa8qacqGHsislcqaHdpWCpaWaaSba aKqbGeaapeGaaGOmaaqcfa4daeqaaaWdbiaawIcacaGLPaaapaWaaW baaeqajuaibaWdbiaaikdaaaqcfaOaey4kaSYaaeWaa8aabaWdbiab eo8aZ9aadaWgaaqcfasaa8qacaaIYaaajuaGpaqabaWdbiabgkHiTi abeo8aZ9aadaWgaaqcfasaa8qacaaIZaaajuaGpaqabaaapeGaayjk aiaawMcaa8aadaahaaqabKqbGeaapeGaaGOmaaaajuaGcqGH9aqpca aIYaGaaGinaiaadsfapaWaaSbaaKqbGeaapeGaam4taaqcfa4daeqa a8qadaqadaWdaeaapeGaeq4Wdm3damaaBaaajuaibaWdbiaaigdaaK qba+aabeaapeGaey4kaSIaeq4Wdm3damaaBaaajuaibaWdbiaaikda aKqba+aabeaapeGaey4kaSIaeq4Wdm3damaaBaaajuaibaWdbiaaio daaKqba+aabeaaa8qacaGLOaGaayzkaaaaaa@6E71@

Stassi d’Alia

( σ 1 σ 3 ) 2 + ( σ 1 σ 2 ) 2 + ( σ 2 σ 3 ) 2 =2( C o T o )( σ 1 + σ 2 + σ 3 )+2 C o T o MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qadaqadaWdaeaapeGaeq4Wdm3damaaBaaajuaibaWdbiaaigda aKqba+aabeaapeGaeyOeI0Iaeq4Wdm3damaaBaaajuaibaWdbiaaio daaKqba+aabeaaa8qacaGLOaGaayzkaaWdamaaCaaabeqcfasaa8qa caaIYaaaaKqbakabgUcaRmaabmaapaqaa8qacqaHdpWCpaWaaSbaaK qbGeaapeGaaGymaaqcfa4daeqaa8qacqGHsislcqaHdpWCpaWaaSba aKqbGeaapeGaaGOmaaqcfa4daeqaaaWdbiaawIcacaGLPaaapaWaaW baaeqajuaibaWdbiaaikdaaaqcfaOaey4kaSYaaeWaa8aabaWdbiab eo8aZ9aadaWgaaqcfasaa8qacaaIYaaajuaGpaqabaWdbiabgkHiTi abeo8aZ9aadaWgaaqcfasaa8qacaaIZaaajuaGpaqabaaapeGaayjk aiaawMcaa8aadaahaaqabKqbGeaapeGaaGOmaaaajuaGcqGH9aqpca aIYaWaaeWaa8aabaWdbiaadoeapaWaaSbaaKqbGeaapeGaam4Baaqc fa4daeqaa8qacqGHsislcaWGubWdamaaBaaajuaibaWdbiaad+gaaK qba+aabeaaa8qacaGLOaGaayzkaaWaaeWaa8aabaWdbiabeo8aZ9aa daWgaaqcfasaa8qacaaIXaaajuaGpaqabaWdbiabgUcaRiabeo8aZ9 aadaWgaaqcfasaa8qacaaIYaaajuaGpaqabaWdbiabgUcaRiabeo8a Z9aadaWgaaqcfasaa8qacaaIZaaajuaGpaqabaaapeGaayjkaiaawM caaiabgUcaRiaaikdacaWGdbWdamaaBaaajuaibaWdbiaad+gaaKqb a+aabeaapeGaamiva8aadaWgaaqcfasaa8qacaWGVbaajuaGpaqaba aaaa@7A8C@

Table 3 Common rock failure criteria

Lithology

Sandstone

Shale

Combo

Limestone

Dolomite

K1

403275

54754

74794

123913

6076

K2

23.87

23.87

23.87

23.87

0

K3

2.35

1.80

1.92

2

1

K4

0

0

0

0.014

20.99

Table 4 Criteria for Normally Occupied Buildings

Rock Mechanical Properties and Rock Strength Determination

The elastic moduli and the mechanical properties of a rock are basic parameters for in-situ stresses and rock strength estimation. Those are calibrated with triaxial tests in laboratory33. However, bulk density (ρb) values of density logs and compressional (ΔtC) and shear slowness (ΔtS) values of sonic dipole logsare utilized together in order to estimate the elastic moduli2:
υ= 1 2 ( Δ t s Δ t c ) 2 1 ( Δ t s Δ t c ) 2 1 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacqaHfpqDcqGH9aqpdaWcaaWdaeaapeWaaSaaa8aabaWdbiaa igdaa8aabaWdbiaaikdaaaWaaeWaa8aabaWdbmaalaaapaqaaGGab8 qacqWFuoarcaWG0bWdamaaBaaajuaibaWdbiaadohaaKqba+aabeaa aeaapeGae8hLdqKaamiDa8aadaWgaaqcfasaa8qacaWGJbaajuaGpa qabaaaaaWdbiaawIcacaGLPaaapaWaaWbaaeqajuaibaWdbiaaikda aaqcfaOaeyOeI0IaaGymaaWdaeaapeWaaeWaa8aabaWdbmaalaaapa qaa8qacqWFuoarcaWG0bWdamaaBaaajuaibaWdbiaadohaaKqba+aa beaaaeaapeGae8hLdqKaamiDa8aadaWgaaqcfasaa8qacaWGJbaaju aGpaqabaaaaaWdbiaawIcacaGLPaaapaWaaWbaaeqajuaibaWdbiaa ikdaaaqcfaOaeyOeI0IaaGymaaaaaaa@5790@ (15)
G= ρ b ( Δ t s ) 2 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacaWGhbGaeyypa0ZaaSaaa8aabaWdbiabeg8aY9aadaWgaaqc fasaa8qacaWGIbaajuaGpaqabaaabaWdbmaabmaapaqaaGGab8qacq WFuoarcaWG0bWdamaaBaaajuaibaWdbiaadohaaKqba+aabeaaa8qa caGLOaGaayzkaaWdamaaCaaabeqcfasaa8qacaaIYaaaaaaaaaa@43B2@ (16)
E=2G( 1+υ ) MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacaWGfbGaeyypa0JaaGOmaiaadEeadaqadaWdaeaapeGaaGym aiabgUcaRiabew8a1bGaayjkaiaawMcaaaaa@3F09@ (17)
K= ρ b ( Δ t s ) 2 4 3 G MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacaWGlbGaeyypa0ZaaSaaa8aabaWdbiabeg8aY9aadaWgaaqc fasaa8qacaWGIbaajuaGpaqabaaabaWdbmaabmaapaqaaGGab8qacq WFuoarcaWG0bWdamaaBaaajuaibaWdbiaadohaaKqba+aabeaaa8qa caGLOaGaayzkaaWdamaaCaaabeqcfasaa8qacaaIYaaaaaaajuaGcq GHsisldaWcaaWdaeaapeGaaGinaaWdaeaapeGaaG4maaaacaWGhbaa aa@47C6@ (18)
λ=K 2 3 G MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacqaH7oaBcqGH9aqpcaWGlbGaeyOeI0YaaSaaa8aabaWdbiaa ikdaa8aabaWdbiaaiodaaaGaam4raaaa@3DAF@ (19)

The rock strength value which is known as the unconfined compressive strength usually termed as UCS or Co can be determined experimentally using core sample18. However, when core samples are not available for laboratory testing, various correlations are performed to estimate the rock value. These correlations that had been developed to predict the uniaxial compressive strength using well log data and predict the rock strength are presented by Zobak's table18. However, Onyia and Andrews34 equations 20 through 21, which are based on sonic log and rock porosity, are widely used In order to estimate the rock strength at any depth because they have acceptable accuracy34,35. In order to reach a higher level of UCS prediction accuracy, Amani and Shahbazi36 new correlation 23, which is employing the porosity in rock strength estimation by using sonic travel time and porosity, is used.

UCS= 1 K 1 ( Δ t c K 2 ) K 3 + K 4 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacaWGvbGaam4qaiaadofacqGH9aqpdaWcaaWdaeaapeGaaGym aaWdaeaapeGaam4sa8aadaWgaaqcfasaa8qacaaIXaaajuaGpaqaba WdbmaabmaapaqaaGGab8qacqWFuoarcaWG0bWdamaaBaaajuaibaWd biaadogaaKqba+aabeaapeGaeyOeI0Iaam4sa8aadaWgaaqcfasaa8 qacaaIYaaajuaGpaqabaaapeGaayjkaiaawMcaa8aadaahaaqabeaa peGaam4sa8aadaWgaaqcfasaa8qacaaIZaaajuaGpaqabaaaaaaape Gaey4kaSIaam4sa8aadaWgaaqcfasaa8qacaaI0aaajuaGpaqabaaa aa@4DDB@ (20)
UCS= 149595( 1 φ 0.18 )f ( Δ t c 40 ) 0.42 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacaWGvbGaam4qaiaadofacqGH9aqpdaWcaaWdaeaapeGaaGym aiaaisdacaaI5aGaaGynaiaaiMdacaaI1aWaaeWaa8aabaWdbiaaig dacqGHsislcqaHgpGApaWaaWbaaeqajuaibaWdbiaaicdacaGGUaGa aGymaiaaiIdaaaaajuaGcaGLOaGaayzkaaGaamOzaaWdaeaapeWaae Waa8aabaacceWdbiab=r5aejaadshapaWaaSbaaKqbGeaapeGaam4y aaqcfa4daeqaa8qacqGHsislcaaI0aGaaGimaaGaayjkaiaawMcaa8 aadaahaaqabKqbGeaapeGaaGimaiaac6cacaaI0aGaaGOmaaaaaaaa aa@5497@ (21)
UCS=194.40.6072Δ t c 646.1φ0.01644Δ t c 2 +8.792φΔ t c MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacaWHvbGaaC4qaiaahofacqGH9aqpcaaIXaGaaGyoaiaaisda caGGUaGaaGinaiabgkHiTiaaicdacaGGUaGaaGOnaiaaicdacaaI3a GaaGOmaGGabiab=r5aejaahshapaWaaSbaaKqbGeaapeGaaC4yaaqc fa4daeqaa8qacqGHsislcaaI2aGaaGinaiaaiAdacaGGUaGaaGymai ab=z8aQjabgkHiTiaaicdacaGGUaGaaGimaiaaigdacaaI2aGaaGin aiaaisdacqWFuoarcaWH0bWdamaaBaaajuaibaWdbiaahogaaKqba+ aabeaadaahaaqabKqbGeaapeGaaGOmaaaajuaGcqGHRaWkcaaI4aGa aiOlaiaaiEdacaaI5aGaaGOmaiab=z8aQjab=r5aejaahshapaWaaS baaKqbGeaapeGaaC4yaaqcfa4daeqaaaaa@6496@ (22)

Where
f=0.0016 d 4 +0.0181 d 3 0.075 d 2 +0.312d+0.5 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacaqGMbGaeyypa0JaeyOeI0IaaGimaiaac6cacaaIWaGaaGim aiaaigdacaaI2aGaaeiza8aadaahaaqabKqbGeaapeGaaGinaaaaju aGcqGHRaWkcaaIWaGaaiOlaiaaicdacaaIXaGaaGioaiaaigdacaqG KbWdamaaCaaabeqcfasaa8qacaaIZaaaaKqbakabgkHiTiaaicdaca GGUaGaaGimaiaaiEdacaaI1aGaaeiza8aadaahaaqabKqbGeaapeGa aGOmaaaajuaGcqGHRaWkcaaIWaGaaiOlaiaaiodacaaIXaGaaGOmai aabsgacqGHRaWkcaaIWaGaaiOlaiaaiwdaaaa@5808@
K1, K2, K3, and K4 are lithology dependent Constants (Table 4)

Time-Based Wellbore Stresses

The induced stresses due to the fluid flow between the wellbore and a permeable formation are presented by Detournay and Cheng37 as shown in equations 23 through 25. In order to express the equations in time domain, a numerical Laplace inversion to the analytical solution of these equations. Stehfest method38 is utilized for this inversion. The induced stresses solutions in time domain are expressed and derived for linear elastic rock deformation to find the fully coupled equations as shown in equations 26.

ΔP r t ~ =( 1 s ) K o ( ξ ) K o ( β ) MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaacceqcfaieaa aaaaaaa8qacqWFuoarcaWHqbGaaCOCa8aadaWgaaqcfasaa8qacaWG 0baajuaGpaqabaWaaWbaaeqabaWdbiaac6haaaGaeyypa0JaeyOeI0 YaaeWaa8aabaWdbmaalaaapaqaa8qacaaIXaaapaqaa8qacaWGZbaa aaGaayjkaiaawMcaamaalaaapaqaa8qacaWGlbWdamaaBaaajuaiba Wdbiaad+gaaKqba+aabeaapeWaaeWaa8aabaWdbiabe67a4bGaayjk aiaawMcaaaWdaeaapeGaam4sa8aadaWgaaqcfasaa8qacaWGVbaaju aGpaqabaWdbmaabmaapaqaa8qacqaHYoGyaiaawIcacaGLPaaaaaaa aa@4F78@ (23)
Δ σ r ~ =2η( P r s )[ R w r K 1 ( ξ ) β K o ( β ) R w 2 r K 1 ( β ) β K o ( β ) ] MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaacceqcfaieaa aaaaaaa8qacqWFuoarcqaHdpWCpaWaa0baaKqbGeaapeGaamOCaaqc fa4daeaapeGaaiOFaaaacqGH9aqpcqGHsislcaaIYaGaeq4TdG2aae Waa8aabaWdbmaalaaapaqaa8qacaWGqbWdamaaBaaajuaibaWdbiaa dkhaaKqba+aabeaaaeaapeGaam4CaaaaaiaawIcacaGLPaaadaWada WdaeaapeWaaSaaa8aabaWdbiaadkfapaWaaSbaaKqbGeaapeGaam4D aaqcfa4daeqaaaqaa8qacaWGYbaaamaalaaapaqaa8qacaWGlbWdam aaBaaajuaibaWdbiaaigdaaKqba+aabeaapeWaaeWaa8aabaWdbiab e67a4bGaayjkaiaawMcaaaWdaeaapeGaeqOSdiMaam4sa8aadaWgaa qcfasaa8qacaWGVbaajuaGpaqabaWdbmaabmaapaqaa8qacqaHYoGy aiaawIcacaGLPaaaaaGaeyOeI0YaaSaaa8aabaWdbiaadkfapaWaa0 baaKqbGeaapeGaam4DaaWdaeaapeGaaGOmaaaaaKqba+aabaWdbiaa dkhaaaWaaSaaa8aabaWdbiaadUeapaWaaSbaaKqbGeaapeGaaGymaa qcfa4daeqaa8qadaqadaWdaeaapeGaeqOSdigacaGLOaGaayzkaaaa paqaa8qacqaHYoGycaWGlbWdamaaBaaajuaibaWdbiaad+gaaKqba+ aabeaapeWaaeWaa8aabaWdbiabek7aIbGaayjkaiaawMcaaaaaaiaa wUfacaGLDbaaaaa@6F29@ (24)
Δ σ θ ~ =2η( P r s )[ R w r K 1 ( ξ ) β K o ( β ) R w 2 r 2 K 1 ( β ) β K o ( β ) + K 1 ( ξ ) K o ( β ) ] MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaacceqcfaieaa aaaaaaa8qacqWFuoarcqaHdpWCpaWaa0baaKqbGeaapeGaeqiUdeha juaGpaqaa8qacaGG+baaaiabg2da9iaaikdacqaH3oaAdaqadaWdae aapeWaaSaaa8aabaWdbiaadcfapaWaaSbaaKqbGeaapeGaamOCaaqc fa4daeqaaaqaa8qacaWGZbaaaaGaayjkaiaawMcaamaadmaapaqaa8 qadaWcaaWdaeaapeGaamOua8aadaWgaaqcfasaa8qacaWG3baajuaG paqabaaabaWdbiaadkhaaaWaaSaaa8aabaWdbiaadUeapaWaaSbaaK qbGeaapeGaaGymaaqcfa4daeqaa8qadaqadaWdaeaapeGaeqOVdGha caGLOaGaayzkaaaapaqaa8qacqaHYoGycaWGlbWdamaaBaaajuaiba Wdbiaad+gaaKqba+aabeaapeWaaeWaa8aabaWdbiabek7aIbGaayjk aiaawMcaaaaacqGHsisldaWcaaWdaeaapeGaamOua8aadaqhaaqcfa saa8qacaWG3baapaqaa8qacaaIYaaaaaqcfa4daeaapeGaamOCa8aa daahaaqabKqbGeaapeGaaGOmaaaaaaqcfa4aaSaaa8aabaWdbiaadU eapaWaaSbaaKqbGeaapeGaaGymaaqcfa4daeqaa8qadaqadaWdaeaa peGaeqOSdigacaGLOaGaayzkaaaapaqaa8qacqaHYoGycaWGlbWdam aaBaaajuaibaWdbiaad+gaaKqba+aabeaapeWaaeWaa8aabaWdbiab ek7aIbGaayjkaiaawMcaaaaacqGHRaWkdaWcaaWdaeaapeGaam4sa8 aadaWgaaqcfasaa8qacaaIXaaajuaGpaqabaWdbmaabmaapaqaa8qa cqaH+oaEaiaawIcacaGLPaaaa8aabaWdbiaadUeapaWaaSbaaKqbGe aapeGaam4Baaqcfa4daeqaa8qadaqadaWdaeaapeGaeqOSdigacaGL OaGaayzkaaaaaaGaay5waiaaw2faaaaa@7E1D@ (25)

Where
η=α ( 1υ ) 2( 1υ ) ,ξ=r s c ,β= R w s c ,c= k μ ( ϕ C t α 2 λ+2G ) MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacqaH3oaAcqGH9aqpcqaHXoqydaWcaaWdaeaapeWaaeWaa8aa baWdbiaaigdacqGHsislcqaHfpqDaiaawIcacaGLPaaaa8aabaWdbi aaikdadaqadaWdaeaapeGaaGymaiabgkHiTiabew8a1bGaayjkaiaa wMcaaaaacaGGSaGaeqOVdGNaeyypa0JaamOCamaakaaapaqaa8qada WcaaWdaeaapeGaam4CaaWdaeaapeGaam4yaaaaaeqaaiaacYcacqaH YoGycqGH9aqpcaWGsbWdamaaBaaajuaibaWdbiaadEhaaKqba+aabe aapeWaaOaaa8aabaWdbmaalaaapaqaa8qacaWGZbaapaqaa8qacaWG JbaaaaqabaGaaiilaiaadogacqGH9aqpdaWcaaWdaeaapeGaam4Aaa WdaeaapeGaeqiVd0gaamaabmaapaqaa8qacqaHvpGzcaWGdbWdamaa BaaajuaibaWdbiaadshaaKqba+aabeaapeWaaSaaa8aabaWdbiabeg 7aH9aadaahaaqabKqbGeaapeGaaGOmaaaaaKqba+aabaWdbiabeU7a SjabgUcaRiaaikdacaWGhbaaaaGaayjkaiaawMcaaaaa@693F@
P rt = P r +( P w P r )ΔP( r,t ) MathType@MTEF@5@5@+= feaagKart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacaWHqbWdamaaBaaajuaibaWdbiaahkhacaWH0baajuaGpaqa baWdbiabg2da9iaahcfapaWaaSbaaKqbGeaapeGaaCOCaaqcfa4dae qaa8qacqGHRaWkdaqadaWdaeaapeGaaCiua8aadaWgaaqcfasaa8qa caWH3baajuaGpaqabaWdbiabgkHiTiaahcfapaWaaSbaaKqbGeaape GaaCOCaaqcfa4daeqaaaWdbiaawIcacaGLPaaaiiqacqWFuoarcaWH qbWaaeWaa8aabaWdbiaahkhacaGGSaGaaCiDaaGaayjkaiaawMcaaa aa@4E73@

σ rr = σ x + σ y 2 ( 1 R w 2 r 2 )+ σ x σ y 2 ( 1+3 R w 4 r 4 4 R w 2 r 2 )cos2θ+ τ xy ( 1+3 R w 4 r 4 4 R w 2 r 2 )sin2θ+ P w R w 2 r 2 +Δ σ r ( r,t ) MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaacceqcfaieaa aaaaaaa8qacqWFdpWCpaWaaSbaaKqbGeaapeGaaCOCaiaahkhaaKqb a+aabeaapeGaeyypa0ZaaSaaa8aabaWdbiab=n8aZ9aadaWgaaqcfa saa8qacaWH4baajuaGpaqabaWdbiabgUcaRiab=n8aZ9aadaWgaaqc fasaa8qacaWH5baajuaGpaqabaaabaWdbiaaikdaaaWaaeWaa8aaba WdbiaaigdacqGHsisldaWcaaWdaeaapeGaaCOua8aadaqhaaqcfasa a8qacaWH3baapaqaa8qacaaIYaaaaaqcfa4daeaapeGaaCOCa8aada ahaaqabKqbGeaapeGaaGOmaaaaaaaajuaGcaGLOaGaayzkaaGaey4k aSYaaSaaa8aabaWdbiab=n8aZ9aadaWgaaqcfasaa8qacaWH4baaju aGpaqabaWdbiabgkHiTiab=n8aZ9aadaWgaaqcfasaa8qacaWH5baa juaGpaqabaaabaWdbiaaikdaaaWaaeWaa8aabaWdbiaaigdacqGHRa WkcaaIZaWaaSaaa8aabaWdbiaahkfapaWaa0baaKqbGeaapeGaaC4D aaWdaeaapeGaaGinaaaaaKqba+aabaWdbiaahkhapaWaaWbaaeqaju aibaWdbiaaisdaaaaaaKqbakabgkHiTiaaisdadaWcaaWdaeaapeGa aCOua8aadaqhaaqcfasaa8qacaWH3baapaqaa8qacaaIYaaaaaqcfa 4daeaapeGaaCOCa8aadaahaaqabKqbGeaapeGaaGOmaaaaaaaajuaG caGLOaGaayzkaaGaci4yaiaac+gacaGGZbGaaGOmaiab=H7aXjabgU caRiab=r8a09aadaWgaaqcfasaa8qacaWH4bGaaCyEaaqcfa4daeqa a8qadaqadaWdaeaapeGaaGymaiabgUcaRiaaiodadaWcaaWdaeaape GaaCOua8aadaqhaaqcfasaa8qacaWH3baapaqaa8qacaaI0aaaaaqc fa4daeaapeGaaCOCa8aadaahaaqabKqbGeaapeGaaGinaaaaaaqcfa OaeyOeI0IaaGinamaalaaapaqaa8qacaWHsbWdamaaDaaajuaibaWd biaahEhaa8aabaWdbiaaikdaaaaajuaGpaqaa8qacaWHYbWdamaaCa aabeqcfasaa8qacaaIYaaaaaaaaKqbakaawIcacaGLPaaaciGGZbGa aiyAaiaac6gacaaIYaGae8hUdeNaey4kaSIaaCiua8aadaWgaaqcfa saa8qacaWH3baajuaGpaqabaWdbmaalaaapaqaa8qacaWHsbWdamaa DaaajuaibaWdbiaahEhaa8aabaWdbiaaikdaaaaajuaGpaqaa8qaca WHYbWdamaaCaaabeqcfasaa8qacaaIYaaaaaaajuaGcqGHRaWkcqWF uoarcqWFdpWCpaWaaSbaaKqbGeaapeGaaCOCaaqcfa4daeqaa8qada qadaWdaeaapeGaaCOCaiaacYcacaWH0baacaGLOaGaayzkaaaaaa@A5E7@

σ θθ = σ x + σ y 2 ( 1 R w 2 r 2 ) σ x σ y 2 ( 1+3 R w 4 r 4 )cos2θ τ xy ( 1+3 R w 4 r 4 )sin2θ P w R w 2 r 2 +Δ σ θ ( r,t ) MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaacceqcfaieaa aaaaaaa8qacqWFdpWCpaWaaSbaaKqbGeaapeGae8hUdeNae8hUdeha juaGpaqabaWdbiabg2da9maalaaapaqaa8qacqWFdpWCpaWaaSbaaK qbGeaapeGaaCiEaaqcfa4daeqaa8qacqGHRaWkcqWFdpWCpaWaaSba aKqbGeaapeGaaCyEaaqcfa4daeqaaaqaa8qacaaIYaaaamaabmaapa qaa8qacaaIXaGaeyOeI0YaaSaaa8aabaWdbiaahkfapaWaa0baaKqb GeaapeGaaC4DaaWdaeaapeGaaGOmaaaaaKqba+aabaWdbiaahkhapa WaaWbaaeqajuaibaWdbiaaikdaaaaaaaqcfaOaayjkaiaawMcaaiab gkHiTmaalaaapaqaa8qacqWFdpWCpaWaaSbaaKqbGeaapeGaaCiEaa qcfa4daeqaa8qacqGHsislcqWFdpWCpaWaaSbaaKqbGeaapeGaaCyE aaqcfa4daeqaaaqaa8qacaaIYaaaamaabmaapaqaa8qacaaIXaGaey 4kaSIaaG4mamaalaaapaqaa8qacaWHsbWdamaaDaaajuaibaWdbiaa hEhaa8aabaWdbiaaisdaaaaajuaGpaqaa8qacaWHYbWdamaaCaaabe qcfasaa8qacaaI0aaaaaaaaKqbakaawIcacaGLPaaaciGGJbGaai4B aiaacohacaaIYaGae8hUdeNaeyOeI0Iae8hXdq3damaaBaaajuaiba WdbiaahIhacaWH5baajuaGpaqabaWdbmaabmaapaqaa8qacaaIXaGa ey4kaSIaaG4mamaalaaapaqaa8qacaWHsbWdamaaDaaajuaibaWdbi aahEhaa8aabaWdbiaaisdaaaaajuaGpaqaa8qacaWHYbWdamaaCaaa beqcfasaa8qacaaI0aaaaaaaaKqbakaawIcacaGLPaaaciGGZbGaai yAaiaac6gacaaIYaGae8hUdeNaeyOeI0IaaCiua8aadaWgaaqcfasa a8qacaWH3baajuaGpaqabaWdbmaalaaapaqaa8qacaWHsbWdamaaDa aajuaibaWdbiaahEhaa8aabaWdbiaaikdaaaaajuaGpaqaa8qacaWH YbWdamaaCaaabeqcfasaa8qacaaIYaaaaaaajuaGcqGHRaWkcqWFuo arcqWFdpWCpaWaaSbaaKqbGeaapeGae8hUdehajuaGpaqabaWdbmaa bmaapaqaa8qacaWHYbGaaiilaiaahshaaiaawIcacaGLPaaaaaa@976A@

σ zz = σ z υ[ 2( σ x σ y ) R w 2 r 2 cos2θ+ τ xy R w 2 r 2 sin2θ ] MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaacceqcfaieaa aaaaaaa8qacqWFdpWCpaWaaSbaaKqbGeaapeGaaCOEaiaahQhaaKqb a+aabeaapeGaeyypa0Jae83Wdm3damaaBaaajuaibaWdbiaahQhaaK qba+aabeaapeGaeyOeI0Iae8xXdu3aamWaa8aabaWdbiaaikdadaqa daWdaeaapeGae83Wdm3damaaBaaajuaibaWdbiaahIhaaKqba+aabe aapeGaeyOeI0Iae83Wdm3damaaBaaajuaibaWdbiaahMhaaKqba+aa beaaa8qacaGLOaGaayzkaaWaaSaaa8aabaWdbiaahkfapaWaa0baaK qbGeaapeGaaC4DaaWdaeaapeGaaGOmaaaaaKqba+aabaWdbiaahkha paWaaWbaaeqajuaibaWdbiaaikdaaaaaaKqbakGacogacaGGVbGaai 4CaiaaikdacqWF4oqCcqGHRaWkcqWFepaDpaWaaSbaaKqbGeaapeGa aCiEaiaahMhaaKqba+aabeaapeWaaSaaa8aabaWdbiaahkfapaWaa0 baaKqbGeaapeGaaC4DaaWdaeaapeGaaGOmaaaaaKqba+aabaWdbiaa hkhapaWaaWbaaeqajuaibaWdbiaaikdaaaaaaKqbakGacohacaGGPb GaaiOBaiaaikdacqWF4oqCaiaawUfacaGLDbaaaaa@6DE6@

τ rθ = σ x σ y 2 ( 1+2 R w 2 r 2 3 R w 4 r 4 )sin2θ+ τ xy ( 13 R w 4 r 4 +2 R w 2 r 2 )cos2θ MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaaccaqcfaieaa aaaaaaa8qacqWFepaDpaWaaSbaaKqbGeaapeGaaCOCaGGabiab+H7a Xbqcfa4daeqaa8qacqGH9aqpdaWcaaWdaeaapeGae43Wdm3damaaBa aajuaibaWdbiaahIhaaKqba+aabeaapeGaeyOeI0Iae43Wdm3damaa BaaajuaibaWdbiaahMhaaKqba+aabeaaaeaapeGaaGOmaaaadaqada WdaeaapeGaaGymaiabgUcaRiaaikdadaWcaaWdaeaapeGaaCOua8aa daqhaaqcfasaa8qacaWH3baapaqaa8qacaaIYaaaaaqcfa4daeaape GaaCOCa8aadaahaaqabKqbGeaapeGaaGOmaaaaaaqcfaOaeyOeI0Ia aG4mamaalaaapaqaa8qacaWHsbWdamaaDaaajuaibaWdbiaahEhaa8 aabaWdbiaaisdaaaaajuaGpaqaa8qacaWHYbWdamaaCaaabeqcfasa a8qacaaI0aaaaaaaaKqbakaawIcacaGLPaaaciGGZbGaaiyAaiaac6 gacaaIYaGae4hUdeNaey4kaSIae4hXdq3damaaBaaajuaibaWdbiaa hIhacaWH5baajuaGpaqabaWdbmaabmaapaqaa8qacaaIXaGaeyOeI0 IaaG4mamaalaaapaqaa8qacaWHsbWdamaaDaaajuaibaWdbiaahEha a8aabaWdbiaaisdaaaaajuaGpaqaa8qacaWHYbWdamaaCaaabeqcfa saa8qacaaI0aaaaaaajuaGcqGHRaWkcaaIYaWaaSaaa8aabaWdbiaa hkfapaWaa0baaKqbGeaapeGaaC4DaaWdaeaapeGaaGOmaaaaaKqba+ aabaWdbiaahkhapaWaaWbaaeqajuaibaWdbiaaikdaaaaaaaqcfaOa ayjkaiaawMcaaiGacogacaGGVbGaai4CaiaaikdacqGF4oqCaaa@7D45@

τ θz =( τ xz sinθ+ τ yz cosθ )( 1+ R w 2 r 2 ) MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaacceqcfaieaa aaaaaaa8qacqWFepaDpaWaaSbaaKqbGeaaiiaapeGae4hUdeNaaCOE aaqcfa4daeqaa8qacqGH9aqpdaqadaWdaeaapeGaeyOeI0Iae8hXdq 3damaaBaaajuaibaWdbiaahIhacaWH6baajuaGpaqabaWdbiGacoha caGGPbGaaiOBaiab=H7aXjabgUcaRiab=r8a09aadaWgaaqcfasaa8 qacaWH5bGaaCOEaaqcfa4daeqaa8qaciGGJbGaai4BaiaacohacqWF 4oqCaiaawIcacaGLPaaadaqadaWdaeaapeGaaGymaiabgUcaRmaala aapaqaa8qacaWHsbWdamaaDaaajuaibaWdbiaahEhaa8aabaWdbiaa ikdaaaaajuaGpaqaa8qacaWHYbWdamaaCaaabeqcfasaa8qacaaIYa aaaaaaaKqbakaawIcacaGLPaaaaaa@5D8B@
τ rz =( τ xz cosθ+ τ yz sinθ )( 1 R w 2 r 2 ) MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaacceqcfaieaa aaaaaaa8qacqWFepaDpaWaaSbaaKqbGeaapeGaaCOCaiaahQhaaKqb a+aabeaapeGaeyypa0ZaaeWaa8aabaWdbiab=r8a09aadaWgaaqcfa saa8qacaWH4bGaaCOEaaqcfa4daeqaa8qaciGGJbGaai4Baiaacoha cqWF4oqCcqGHRaWkcqWFepaDpaWaaSbaaKqbGeaapeGaaCyEaiaahQ haaKqba+aabeaapeGaci4CaiaacMgacaGGUbGae8hUdehacaGLOaGa ayzkaaWaaeWaa8aabaWdbiaaigdacqGHsisldaWcaaWdaeaapeGaaC Oua8aadaqhaaqcfasaa8qacaWH3baapaqaa8qacaaIYaaaaaqcfa4d aeaapeGaaCOCa8aadaahaaqabKqbGeaapeGaaGOmaaaaaaaajuaGca GLOaGaayzkaaaaaa@5BEA@

Wellbore Stability Model flow diagram

Figure 1 shows a flow diagram of the wellbore instability developed model procedures. It include four main parts: building MEM, time-based wellbore stress analysis, safe mud weight determination, and wellbore trajectory optimization.

Figure 1 Wellbore instability developed model flow diagram. "/>

Figure 1 Wellbore instability developed model flow diagram.

Case Studies and Model Validation

Well RBS-91 Description

Well RBS-91 is a directional well, located within RBS-9 field in Romania. The well area is located in the central north-Eastern of a rift system margin. The main structures of this area are horsts, grabens, and faults striking NW-SE. This basin is described a highly active tectonic area, which lead to a high anisotropy in the horizontal stresses. The dataset of the well logs that have been recorded during the drilling phase of the well, includes cross dipole sonic log, neutron porosity log, density log and 6-arm caliper log as shown in Figures (2&3). After examining these logs, it is clearly observed that there are severe breakouts in the 8½ inch hole section as appeared in Figure (3).

Figure 2 Composite log for well RBS-91. "/>

Figure 2 Composite log for well RBS-91.

Figure 3 (a) 3D wellbore image and cross section for well RBS-91, instability zone using6-arm caliper log
(b). Determination of σhmax using breakout analysis for instability zone. "/>

Figure 3 (a) 3D wellbore image and cross section for well RBS-91, instability zone using6-arm caliper log
(b). Determination of σhmax using breakout analysis for instability zone.

Developed Model Analysis for Well RBS-91

In order to perform an excellent analysis and validate the developed model, the MEM is firstly developed for instability zones (3650 m – 3800 m) of well RBS-91 as illustrated in the preceded flow diagram. The MEM results for wellbore instability zone which include overburden stress (sv), minimum horizontal stress (sh), maximum horizontal stress (sh), bulk modulus (K), shear modulus (G), Young's modulus (E), Poisson's ratio (υ),pore pressure (Pp), and uniaxial compressive strength (UCS) are shown in Figure (4). The developed model shows that the maximum shear stress around the wellbore is at 63º and 243º counterclockwise for a long time period (30 hrs) after drilling this zone (Figure 5). The shear stress curves at different times are overlaid and reached the maximum value instantaneously at the wellbore wall (r/rw=1) for all time periods. However, the alteration of hoop stress and the time dependency are significantly realized when the radial distance (r) increases more than (rw). The shear stress curves at various times periods become separated and the effect of time appears (Figure 6). Additionally, Figure (7) shows the shear stress alteration for 4 time periods versus the radial distance from the wellbore at θ=63º. It’s clearly observed that the shear stress has a maximum constant value at the wellbore wall, a significant difference around borehole wall, and becomes identical far away from wellbore wall. That means the stress magnitude decreases as the radial distance from the wellbore increases, until it reaches the value of the in-situ maximum horizontal stress. Obviously, the shear stresses increase with time and may extend the shear failure if it goes beyond the value of the rock strength. However, the failure will never be initiated with time as it is mentioned above that the shear stress value has reached at the wellbore wall instantaneously to its maximum after drilling the formation.

Figure 4 The MEM resultsof developed model for Well RBS-91. "/>

Figure 4 The MEM resultsof developed model for Well RBS-91.

Figure 5 The MEM resultsof developed model for Well RBS-91. "/>

Figure 5 The poroelastic model tangential stresses as a function of inclination and time at r/Rw=1.

Figure 6 The poroelastic model tangential stresses as a function of inclination and time at r/Rw=1.1. "/>

Figure 6 The poroelastic model tangential stresses as a function of inclination and time at r/Rw=1.1.

Figure 7 The poroelastic model tangential stresses as a function of inclination and time at r/Rw=1.1. "/>

Figure 7 The poroelastic model tangential stresses as a function of radial distance and time.

The developed model also shows radial stress variations with the radial distance from the wellbore for the same time periods (Figure 8). The radial stress is identical to the wellbore pressure at the wellbore walls. Moving far from the wellbore, the radial stress starts to increase until it reaches the minimum in-situ horizontal stress. Moreover, Figure (9) shows pore pressure changes with respect to time and radial distance. The pore pressure is the same as the wellbore pressure once the formation is opened at the wellbore wall. Since the wellbore pressure is higher than the pore pressure (overbalance drilling), the drilling fluid invades the formation and the formation pressure starts to increase with time.

Figure 8 The poroelastic model radial stresses as a function of radial distance and time. "/>

Figure 8 The poroelastic model radial stresses as a function of radial distance and time.

Figure 9 The poroelastic model pore pressure as a function of radial distance and time. "/>

Figure 9 The poroelastic model pore pressure as a function of radial distance and time.

In order to validate the effectiveness of the developed model, the actual mud weight, azimuth, and inclination for instability zones (3650 m – 3800 m) are utilized. The developed model results for actual and calculated ones are compared together. The model shows the radial and the shear stresses as well as the failure and the pore pressure profiles (rows) at various time periods (columns) for instability zones (Figure 10). The first row represents the radial stresses, the second is the shear stresses, the third is the failure profile and the last row is the pore pressure profile. Obviously, the propagation of shear failure is changed with time. Additionally, Figure 10 is a contour representation for shear failure index (Isf) - predicting failure obviously reduces itself to comparing the internal stresses (s) to the material’s strength in the loading direction- around the wellbore at time periods 0, 1, 15, and 60 minutes. This figure is a perfect representation of the Isf which can predict the shape and the size of the shear failure of the wellbore. The blue area represents Isf < 0 hence, shear failure will take place, while the yellow area and the yellow shade represents area represents Isf > 0, hence, no shear failure. According to the developed model, a minor shear failure that will take place onset drilling is predicted. However, after 60 minutes, the model predicts that the shear failure will extend as shown in Figure 10. Comparing this result with the actual wellbore image log (Figure 3), a good match between the caliper log and failure prediction done by the developed model is observed and achieved. Therefore, the developed model has higher accuracy than the linear elastic model.

Figure 10 Stresses and failure profiles as a function of time for instability zones. "/>

Figure 10 Stresses and failure profiles as a function of time for instability zones.

The safe mud pressure window as a function of the wellbore inclination angle is predicted with the modified Lade failure criterion which is selected because it is the most common and accurate criterion in petroleum industry based on the published studies (Figure11). The red color represents a fracture region, the green color shows a safe region and the blue color indicates a collapse region. The bright color star represents the RBS-91 wellbore conditions (inclination, borehole pressure) which is located inside the collapse region. In Figure 11, it is observed that the safe pressure window is very narrow at the high deviation angle at the current well azimuth (240º). In order to resolve this failure, the mud weight should, therefore, be increased or the well inclination should be changed. As in Figure 11, if the well inclination is selected to be changed, the wellbore mud density will also vary in order to keep the well in safe window during drilling this unstable zone in future developments.

Figure 11 Mud pressure window function of inclination angle for instability zones. "/>

Figure 11 Mud pressure window function of inclination angle for instability zones.

In order to remedial and mitigate the breakout failure problem associated with instability zones in the future wells, the following suggestions are recommended for remedial:

  1. Optimize the borehole pressure (Increase the mud weight)
  2. Optimize the wellbore trajectory (Adjust the azimuth and the inclination)
  3. Optimize both of borehole pressure and trajectory

For wellbore pressure optimization, the developed model optimizes the mud weight required to tackle instability problem using the most common failure criterion in petroleum industry (Modified Lade). It shows that the minimum and maximum safe mud weight in order to avoid shear and tensile failure are 9.8 and 15.5 ppg respectively (Figure 12). This is because 9.8 and 15.5 ppg represent the minimum and the maximum safe curves for instability zone. However, the wellbore trajectory optimization is shown in Figure 13 a through d in which a stereo net map is representing the shear failure index (Isf) as a function of wellbore azimuth and inclination. The color map of the plot indicates how far the well is away from the shear failure, blue is the safest region, and red is a failure region. The actual wellbore trajectory is represented with the black circle on the map. Obviously, the wellbore stability cannot be maintain with the current mud weight for any well trajectory, therefore the wellbore trajectory optimization is not enough to avoid the wellbore failure. As a result, this solution is not applicable. Changing the mud weight with alternating wellbore inclination and azimuth would result in selecting the optimum trajectory. The more the mud weight, the safer wellbore trajectory is shown and the more easy to drill this section without collapse failure using different wellbore trajectories (Figure13). However, there is a limit for increasing the mud weight to avoid fracture the formation. Therefore, the optimum wellbore trajectory that can be drilled safely utilizing the minimum mud weight should be determined. Optimization of borehole pressure and well trajectory is then required. The minimum required mud weight to prevent shear failure and the maximum required mud weight to avoid tensile failure as a function of wellbore azimuth and deviation angles are presented in Figure (13e&f). As an overview on the relationship between the wellbore trajectory and the optimum mud weight, this well section obviously cannot be drilled horizontally in direction of the minimum horizontal stress (Azimuth = 60º) due to the narrow allowable mud window.

Figure 12 Modified Lade criterion function of wellbore pressure for Instability zone. "/>

Figure 12 Modified Lade criterion function of wellbore pressure for Instability zone.

Figure 13 (a, b, c, d) The model shear failure index projection on Stereo net map function of inclination and azimuth Mwt 9.2 ppg, 10.2 ppg, 11.2 ppg, and 12.2 pp respectively.(e, f)Minimum and maximum allowable mud weight as function of well inclination and azimuth respectively. "/>

Figure 13 (a, b, c, d) The model shear failure index projection on Stereo net map function of inclination and azimuth Mwt 9.2 ppg, 10.2 ppg, 11.2 ppg, and 12.2 pp respectively.(e, f)Minimum and maximum allowable mud weight as function of well inclination and azimuth respectively.

Conclusions and Recommendations

A time-dependent developed model for wellbore instability prediction was implemented in this article. The developed model is effectively predicting the safe mud weight window and optimizing the wellbore trajectory. Based on the results and analysis, the following conclusions and recommendations are extracted:

  1. Well bore instability are predicted utilizing available well log and drilling data without available core measurements.
  2. The developed model is successful for predicting instability zones
  3. The failure criteria with the effect of intermediate principal stress show an effective way for rock failure description in the developed model more than those which are not considered the intermediate principal stress.
  4. The poroelastic model yielded better accuracy to predicting wellbore failure with time.
  5. The mitigation of wellbore instability can be performed by increasing the mud weight or orienting the wellbore to different direction. However, in some cases, the change in wellbore trajectory is not enough and mud weight must be increased.
  6. The developed wellbore instability model is potentially applicable to other field cases using a similar approach which could be adjusted to the particular field specifications and requirements.

Nomenclatures
as, bs = Rock coefficient values
c = generalized consolidation coefficient (Diffusion coefficient)
Co= Unconfined compressive strength of rock (Uniaxial Compressive strength),
C'2, C'1=Constants calculated by the rock properties at the test depth
ct= rock total compressibility which is equal to the inverse of the Bulk modulus of elasticity K.
d = depth in km
E = Young’s modulus
G = Shear modulus
g = gravitational acceleration.
h= depth, ft.
k = absolute permeability
K= Bulk Modulus
𝐾0, 𝐾1 = zero and the first order of modified Bessel function of the second kind
Pe=Pressure difference between minimum horizontal stress and pore pressure of formation.
Pp= Pore pressure, psi
Pr= pore pressure,
Prn =normal pore pressure which equivalent to vertical height of a column of water along from the surface to the formation of interest
Sh=Minimum horizontal stress from the test data,
r= position radially outwards from the center
Rw, r =Wellbore radius and the radius of investigation
x = an exponent
αb= Biot Coefficient
β = Angle of fault plan, degrees=𝜋/4 – 𝜙/2
γ = the borehole inclination from vertical, degrees
Δtc = sonic compressional travel time in μsec/m
Δtlog= observed acoustic travel time from the sonic log
Δtnorm = normal acoustic travel time
λ = Lame’s Parameter
μ = fluid viscosity
(h) = the density of the rock at depth (h)
ρb= Bulk density for rock, lb/ft.3
σtec=Additional tectonic stress
sv= Overburden stress, psi
sH= Maximum horizontal stress, psi
sh= Minimum horizontal stress, psi
υ= Poisson’s ratio
q= angle with the direction of the maximum horizontal stress
= porosity of rock, fraction
MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacqGHfiIXaaa@381E@ = Internal friction angle
φthe geographical azimuthand the borehole position from the x-axis, q.
𝑣𝑠𝑙𝑜𝑤, 𝑣𝑓𝑎𝑠𝑡 =Poisson’s ratios using the slow shear and fast shear travel time respectively.
S,1=Parameters of failure criterion function of the cohesion of the rock (Co) and internal friction angle () MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaieaaaaaa aaa8qacaGGOaGaeyybIySaaiykaaaa@3977@
η MathType@MTEF@5@5@+= feaagKart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqcfaOaeq4TdG gaaa@3830@ = poroelastic coefficient

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