1
CONCLUSIONS RESERVOIR CONNECTIVITY AND COMPARTMENT BOUNDARIES Bohling, G.C., J. H. Doveton, W. Guy, W.L. Watney, and S. Bhattacharya, 1998, PfEFFER 2.0 manual, Kansas Geological Survey, Lawrence, Kansas, 161 pp. French, V. L., and C. Kerans, 2004, Accommodation-controlled systems-tract-specific facies partioning and resulting geometric development of reservoir grainstone ramp-crest shoal bodies, in Integration of outcrop and modern analogs in reservoir modeling: AAPG Memoir 80, p. 171- 190. Kerans, C., F. J. Lucia, and R. K. Senger, 1994, Integrated characterization of carbonate ramp reservoirs using Permian San Andres Formation outcrop analogs, AAPG Bulletin, v. 78, p. 181-216. Ruppel, S. C., and D. G. Bebout, 2001, Competing effects of depositional architecture and diagenesis on carbonate reservoir development: Grayburg Formation, South Cowden field, west Texas: The University of Texas atAustin, Bureau of Economic Geology Report of Investigations No. 263, 62 p. Ward, R. F., C. G. St. C. Kendall, and P. M. Harris,1986, Upper Permian (Guadalupian) facies and their association with hydrocarbons-- Permian Basin, west Texas and New Mexico: AAPG Bulletin, v. 70, p. 239-262. References iCharlotte Sullivan, Chuck Blumentritt, Kurt Marfurt, and Qifeng Dou, for seismic attribute generation and geological insight i i i i i Burlington Resources Oil & Gas Company and Schlumberger IPM, for providing seismic and well data The U. S. Department of Energy, for project funding under contract DE-FC26-04NT15504 Seismic Micro-Technology, Inc., for access to seismic-interpretation software Hampson-Russell, for access to seismic inversion software IHS, for access to well-log correlation and mapping software The KINGDOM Suite+ STRATA PETRA Acknowledgments BVW profiles from base anhydrite to "x" marker -800 -780 -760 -740 -720 -700 -680 -660 0 0.05 0.1 0.15 BVW Elevationn (ft) 1202w 1261w 1201w 1205w 1206w 1207w 1208w 1209w 1228w 1229w -680 BVW -700 BVW -720 BVW -740 BVW -760 BVW -780 BVW Bubble maps of BVW at a given elevation (subsea in feet) are superimposed on the top of San Andres subsea depth map. These maps show a range in BVW values that are not closely tied to elevation on top of the San Andres Formation. Moreover, values vary markedly by depth in an individual well, reflecting the variation of porosity in the cyclic packstone-grainstone interval.The depth slices also do not show any pattern of BVW variation with depth, paralleling the BVW vs. depth plot above. This lack of depth pattern indicates that there is not a strong field-wide transition zone, but rather local well-scale variations in reservoir properties. i i i i i i i i i i A wide range of fluid recoveries is noted in wells in the “high volume areaof Waddell Field. Higher production generally comes from 1) the main structural high, 2) along the northeast flank of the southeast-trending anticline that runs through the area, and 3) along a narrow northeast-trending area roughly corresponding to a structural saddle on the anticline. In the high volume area, tight, anhydritic macrokarst at the top of the San Andres Formation cuts down into the underlying porous reservoir. The karst zone exhibits high variability in thickness but is generally thicker on the higher portions of the southeast-trending anticline. The porous carbonate reservoir interval below the karst is on the saddle area of the anticline. A seismic horizon corresponding to thexmarker (base of porous reservoir) can be interpreted across the impedance volume. This horizon is truncated by the base of karst in some areas, suggesting an associated change in reservoir type/quality in these areas. A comparison of mean and center of gravity measures of porosity indicates that higher porosity is developed lower in the pay interval. The mean seismic impedance of the reservoir interval corresponds well with mean porosity from well logs and allows porosity approximation in areas of poor well control. The impedance maps suggest that the porous San Andres shoals that comprise the pay appear to have N-NE trends, oblique to the main San Andres structure.The pattern of shoal development may be controlled by deep- seated structure. Local karst development appears to be at a well scale, greatly reducing the reservoir quality, which causes variability in oil and gas production, even within this high volume area A combination of factors appears to be responsible for the pay distribution in the high volume area of Waddell Field. locally thin BVW ANALYSIS Phi-BVW depth profiles (left) of wells #1228 and adjacent #1207 are on opposing ends of the depth cluster. Well #1228 is more tightly clustered at lower values at greater depth due the presence of thick karst, while the phi-BVW points associated with well #1207 are noticeably higher at higher elevations. While both wells are essentially the same elevation at the top of San Andres, as can be seen in the map below, the deeper karst at the location of well #1228 leaves pay in the packstone-grainstone facies at greater depths. The contrast in location of the porous interval in these two wells can be observed in the cross section on the right. -810 -790 -770 -750 -730 -710 -690 -670 -650 0 0.05 0.1 0.15 Phi-BVW Elevation (ft) 1202_phi-bvw 1261_phi-bvw 1201_phi-bvw 1205_phi-bvw 1206_phi-bvw 1207_phi-bvw 1208_phi-bvw 1209_phi-bvw 1228_phi-bvw Well 1207- High elevation and high sum (phi-BVW) Well 1228 - High elevation, offsetting well 1207 and relatively low sum (phi-BVW) 4.18 4.85 7.60 2.18 5.12 2.98 3.69 4.32 1.07 7.77 1229 (not plotted) Sum (Phi-BVW) Top San Andres Phi-BVW for Selected Wells Elevation of lowermost pay Observations of the Phi-BVW depth profile plot: Well #1261 is nearly the lowest in elevation and has the smallest cumulative Phi- BVW of 1.07. Well #1202 is adjacent to well #1261 and at the same elevation at the top of the San Andres, as seen in the map at right. However, the pay interval in #1202 occurs at a higher elevation due to thinner overlying karst. The additional pay interval and higher elevation apparently led to a relatively high cumulative phi- BVW of 4.32 vs. 1.07. Well #1205, near well #1208, has the lowest top of San Andres, but pay is relatively high and cumulative phi-BVW is moderately elevated, 5.12, compared to 2.98. Phi-BVW profiles are similar in pattern, but elevation of pay in #1205 is higher due to less deeply penetrating karst. Thus i i i Structure map top of San Andres Formation. Bubbles depict cumulative Phi-BVW in the pay intervals of each well. Phi-BVW is an indication of hydrocarbon pore volume. No clear pattern is noted, including offset wells with large contrast in pay and structurally low wells with higher pay calculations. Maps of cumulative oil and gas production in the “high volume area” show similar variation on a well-to-well level. 1261 1205 1202 1207 1228 1229 1201 1206 1209 1208 Phi-BVW = hydrocarbon pore volume additional section is available for hydrocarbon accumulation. Well #1228 is located adjacent to well #1207 in a structurally high position on the top of the San Andres, but the pay interval is around 35 feet lower. The phi-BVW profiles are in sharp contrast to one another, 7.77 (one of the highest values) vs. 3.69. Additionally, the maximum pay values (phi-BVW) for individual points decline from 0.1 to 0.5 in well #1228, as indicated by the orange dashed line in the phi-BVW depth plot. Other wells follow this trend of phi-BVW decline with depth suggesting a decline in hydrocarbon saturation, perhaps an indication of transition. Most of the indications of pay (phi-BVW), other than in well #1261, reside at elevations above -788 feet. This may be an indication of the proximity of an oil/water contact. i i PHI-BVW ANALYSIS GENERAL OBSERVATIONS OF PHI-BVW PLOTS AND MAPPING After petrophysical cut-offs are applied and the pay intervals of reservoir are identified, effective porosity can be subtracted from the BVW, the bulk volume water, to estimate hydrocarbon pore volume. Displaying a depth profile of phi-BVW can provide an indication of a hydrocarbon transition zone, where values decrease with depth, eventually dropping to zero at the hydrocarbon/water contact. Similarly, widespread scattering of points with no pattern reveals complex heterogeneity with no transition zone or oil or gas water contact. The phi-BVW depth plot shows some vague patterns related to local reservoir heterogeneity that appears to be developed at the well scale, related to the strong karst overprinting that has generally reduced the more continuous pay developed in the overlying grainstone-packstones. Thus, karst diagenesis pays a significant role in the heteogeneity in the high volume area. Well-scale heterogeneity is similarly reflected in the cumulative production and seismic attribute data. Seismic attribute analysis suggests an element of structural control on this heterogeneity. Low mean impedance in the reservoir interval has been shown to correspond generally to high mean porosity. However, lower mean impedance also appears to correlate with lower cumulative hydrocarbon pore volume from Phi-BVW, as is shown by wells #1261 and #1228 (which have a thicker karst zone), compared to wells #1202 and #1228 (which have a thinner karst zone). This correspondence between high porosity and low hydrocarbon pore volume is most likely explained by the fact that the high porosity is developed deeper in the reservoir interval (as was indicated by the center of gravity map) and in areas with thicker karst, the lower porosity upper reservoir will be cut out, so that only the deeper high porosity interval will contribute to the mean porosity. A most positive curvature map (showing antiform bending) extracted from the seismic data volume along a Devonian horizon approximately 0.6 seconds below the San Andres shows that there is a significant deep-seated structural control to the northwest-trending features in the high volume area. As can be seen by the interleaved most positive curvature and mean reservoir interval impedance maps, there is also an indication that crosscutting north to northeast-trending features on the Devonian surface also impacted porosity development in the San Andres. A most positive curvature map extracted along the xmarker shows some of the same structural trends as the Devonian horizon but also shows a finer network of lineaments that enclose areas with diameters on the order of 1500 ft (450 m). These features may indicate reservoir compartmentalization at a single- well scale. SEISMIC ATTRIBUTE ANALYSIS Most positive volumetric curvature extracted along the “x” marker horizon superimposed on the mean impedance map for the base karst to “x” marker interval. Black corresponds to tight positive (antiformal) curvature. Most positive volumetric curvature extracted along a Devonian horizon (approximately 0.6 seconds below the San Andres) superimposed on the mean impedance map for the base karst to “x” marker interval. Black corresponds to tight positive (antiformal) curvature. 1207 1228 1261 1202 1207 1228 1261 1202

SEISMIC ATTRIBUTE ANALYSIS - Kansas Geological Survey · BVW ANALYSIS Phi-BVW depth profiles (left) of wells #1228 and adjacent #1207 are on opposing ends of the depth cluster. Well

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Page 1: SEISMIC ATTRIBUTE ANALYSIS - Kansas Geological Survey · BVW ANALYSIS Phi-BVW depth profiles (left) of wells #1228 and adjacent #1207 are on opposing ends of the depth cluster. Well

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UN

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RIE

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Bo

hlin

g, G

.C., J

. H. D

oveto

n, W

. Gu

y, W.L

. Watn

ey, a

nd S

. Bhatta

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998, P

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ansas G

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Ka

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nch, V

. L., a

nd C

. Kera

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004,A

ccom

mod

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lled s

yste

ms-tra

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pecific

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eom

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develo

pm

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serv

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mp

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Inte

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tion o

f outc

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nd m

od

ern

analo

gs in

reserv

oir m

odelin

g:A

AP

G M

em

oir 8

0, p

. 171-

190.

Ke

rans, C

., F. J

. Lucia

, and R

. K. S

enger, 1

994

, Inte

gra

ted c

hara

cte

riza

tion o

f carb

onate

ram

p re

serv

oirs

usin

g P

erm

ian S

an

Andre

sF

orm

atio

n o

utc

rop a

nalo

gs,A

AP

G B

ulle

tin, v. 7

8, p

. 181-2

16.

Ru

ppel, S

. C., a

nd D

. G. B

ebout, 2

001, C

om

pe

ting e

ffects

of d

epositio

nal a

rch

itectu

re a

nd d

iagenesis

on c

arb

onate

reserv

oir d

evelo

pm

ent:

Gra

yburg

Fo

rmatio

n, S

outh

Cow

den fie

ld, w

estTexas:T

he U

niv

ers

ity o

fTe

xas a

tA

ustin

, Bure

au o

f Econom

ic G

eo

logy R

eport o

fIn

vestig

atio

ns N

o. 2

63, 6

2 p

.

Wa

rd, R

. F., C

. G. S

t. C. K

endall, a

nd P

. M. H

arris

,1986, U

pper P

erm

ian (G

uadalu

pia

n) fa

cie

s a

nd th

eir a

ssocia

tion w

ith h

ydro

carb

ons--

Pe

rmia

n B

asin

, westTexas a

nd N

ew

Me

xic

o:A

AP

G B

ulle

tin, v. 7

0, p

. 239-2

62.

Refe

ren

ces

iC

harlo

tte S

ulliv

an, C

huck B

lum

entritt, K

urt M

arfu

rt, and Q

ifeng D

ou, fo

r se

ism

ic a

ttribute

genera

tion a

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eolo

gic

al in

sig

ht

iiiii

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rlingto

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om

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chlu

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M, fo

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ata

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. S. D

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icro

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r access to

se

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oftw

are

IHS

, for a

ccess to

well-lo

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appin

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Th

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M S

uite

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PE

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A

Ac

kn

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led

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Wp

rofile

sfro

mb

ase

an

hyd

riteto

"x"m

ark

er

-800

-780

-760

-740

-720

-700

-680

-660

00.0

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W

Elevationn (ft)

1202w

1261w

1201w

1205w

1206w

1207w

1208w

1209w

1228w

1229w

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VW

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VW

Bu

bb

le m

ap

s o

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t a g

ive

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(su

bse

a in

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su

pe

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ose

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p o

f Sa

nA

nd

res s

ub

se

a d

ep

th m

ap

.T

he

se

ma

ps s

ho

w a

ran

ge

in B

VW

va

lue

s th

at a

re n

ot c

lose

ly tie

d to

ele

va

tion

on

top

of th

e S

an

An

dre

s F

orm

atio

n. M

ore

ove

r, va

lue

s v

ary

ma

rke

dly

by d

ep

th in

an

ind

ivid

ua

l we

ll, refle

ctin

g th

e v

aria

tion

of p

oro

sity

in th

e c

yclic

pa

cksto

ne

-gra

insto

ne

inte

rva

l.Th

ed

ep

th s

lice

s a

lso

do

no

t sh

ow

an

y p

atte

rn o

f BV

W v

aria

tion

with

de

pth

, pa

ralle

ling

the

BV

W v

s.

de

pth

plo

t ab

ove

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his

lack o

f de

pth

pa

ttern

ind

ica

tes th

at th

ere

is n

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stro

ng

field

-wid

etra

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on

e, b

ut ra

the

r loca

l we

ll-sca

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aria

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rese

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ir pro

pe

rties.

iiiiiiiiii

Aw

ide

range o

f fluid

recoverie

s is

note

d in

wells

in th

e“h

igh v

olu

me a

rea

”of W

addell F

ield

. Hig

her p

roductio

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m 1

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ain

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nh

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ickness b

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ars

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addle

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horiz

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orre

spondin

g to

the

”x”

mark

er (b

ase o

f poro

us re

serv

oir) c

an b

e in

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rete

d a

cro

ss th

eim

peda

nce v

olu

me.T

his

horiz

on is

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d b

y th

e b

ase o

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t in s

om

e a

reas, s

uggestin

g a

n a

ssocia

ted

change

in re

serv

oir ty

pe/q

uality

in th

ese a

reas.

Acom

paris

on o

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nd c

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r of g

ravity

measure

s o

f poro

sity

indic

ate

s th

at h

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sity

is d

evelo

ped

low

er in

the p

ay in

terv

al.

The m

ean s

eis

mic

impedance o

f the

reserv

oir in

terv

al c

orre

spon

ds w

ell w

ith m

ean p

oro

sity

from

well lo

gs a

nd

allo

ws p

oro

sity

appro

xim

atio

n in

are

as o

f poor w

ell c

ontro

l.

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pedance m

aps s

uggest th

at th

e p

oro

us S

an

Andre

s s

hoa

ls th

at c

om

pris

e th

e p

ay a

ppe

ar to

have N

-NE

trends, o

bliq

ue to

the m

ain

San

And

res s

tructu

re.T

he p

atte

rn o

f shoal d

evelo

pm

ent m

ay b

e c

ontro

lled b

y d

eep-

seate

d s

tructu

re.

Local k

ars

t develo

pm

ent a

ppears

to b

e a

t a w

ell s

cale

, gre

atly

reducin

g th

e re

serv

oir q

uality, w

hic

h c

auses

varia

bility

in o

il and g

as p

roductio

n, e

ven w

ithin

this

hig

h v

olu

me

are

a

Acom

bin

atio

n o

f facto

rs a

ppears

to b

e re

sponsib

le fo

r the p

ay d

istrib

utio

n in

the h

igh v

olu

me

are

a o

f Waddell

Fie

ld.

locally

thin

BV

WA

NA

LY

SIS

Ph

i-BV

W d

ep

th p

rofile

s (le

ft) of w

ells

#1

22

8 a

nd

ad

jac

en

t #1

20

7 a

re o

n o

pp

os

ing

en

ds

of th

e d

ep

th c

lus

ter.

We

ll #1

22

8 is

mo

re tig

htly

clu

ste

red

at lo

we

r va

lue

s a

t gre

ate

r de

pth

du

e th

e p

res

en

ce

of th

ick

ka

rst, w

hile

the

ph

i-BV

W p

oin

ts a

ss

oc

iate

d w

ith w

ell #

12

07

are

no

tice

ab

ly h

igh

er a

t hig

he

r ele

va

tion

s. W

hile

bo

th w

ells

are

es

se

ntia

lly th

e s

am

e e

lev

atio

n a

t the

top

of S

an

An

dre

s, a

s c

an

be

se

en

in th

e m

ap

be

low

, the

de

ep

er k

ars

t at

the

loc

atio

n o

f we

ll #1

22

8 le

av

es

pa

y in

the

pa

ck

sto

ne

-gra

ins

ton

e fa

cie

s a

t gre

ate

r de

pth

s. T

he

co

ntra

st in

loc

atio

n o

f the

po

rou

s in

terv

al in

the

se

two

we

lls c

an

be

ob

se

rve

d in

the

cro

ss

se

ctio

n o

n th

e rig

ht.

-81

0

-79

0

-77

0

-75

0

-73

0

-71

0

-69

0

-67

0

-65

0

00

.05

0.1

0.1

5

Ph

i-BV

W

Elevation (ft)

12

02

_p

hi-b

vw

12

61

_p

hi-b

vw

12

01

_p

hi-b

vw

12

05

_p

hi-b

vw

12

06

_p

hi-b

vw

12

07

_p

hi-b

vw

12

08

_p

hi-b

vw

12

09

_p

hi-b

vw

12

28

_p

hi-b

vw

Well 1

207- H

igh

ele

vatio

n a

nd

hig

h s

um

(ph

i-BV

W)

Well 1

228 - H

igh

ele

vatio

n, o

ffsettin

g w

ell 1

207

an

d re

lativ

ely

low

su

m (p

hi-B

VW

)

4.1

8

4.8

5

7.6

0

2.1

8

5.1

2

2.9

8

3.6

9

4.3

2

1.0

7

7.7

7

1229

(no

t plo

tted

)

Sum (Phi-BVW)

To

p S

an

An

dre

s

Ph

i-BV

W fo

r Se

lec

ted

We

lls

Ele

va

tion

of lo

we

rmo

st

pa

y

Ob

serv

atio

ns o

f the P

hi-B

VW

dep

th p

rofile

plo

t:

Well #

1261 is

nearly

the

low

est in

ele

vatio

n a

nd h

as

the s

malle

st c

um

ula

tive P

hi-

BV

W o

f 1.0

7.

Well #

1202 is

adja

ce

nt to

we

ll#1261 a

nd a

t the s

am

eele

vatio

n a

t the to

p o

f the S

an

Andre

s, a

s s

een in

the m

ap a

trig

ht. H

ow

eve

r, the p

ay

inte

rva

l in #

12

02 o

ccurs

at a

hig

her e

levatio

n d

ue to

thin

ner

overly

ing k

ars

t.T

he a

dditio

nal

pay in

terv

al a

nd h

igh

er

ele

vatio

n a

ppa

rently

led to

are

lativ

ely

hig

h c

um

ula

tive p

hi-

BV

W o

f 4.3

2 v

s. 1

.07

.

Well #

1205, n

ear w

ell #

1208

,has th

e lo

west to

p o

f San

Andre

s, b

ut p

ay is

rela

tively

hig

h a

nd c

um

ula

tive p

hi-B

VW

is m

od

era

tely

ele

vate

d, 5

.12

,com

pa

red to

2.9

8. P

hi-B

VW

pro

files a

re s

imila

r in p

atte

rn,

but e

levatio

n o

f pay in

#1205

is h

igh

er d

ue to

less d

eeply

penetra

ting k

ars

t.T

hus

iii

Stru

ctu

re m

ap

top

of S

an

An

dre

s F

orm

atio

n. B

ub

ble

sd

ep

ict c

um

ula

tive

Ph

i-BV

W in

the

pa

y in

terv

als

of e

ac

hw

ell. P

hi-B

VW

is a

n in

dic

atio

n o

f hy

dro

ca

rbo

n p

ore

vo

lum

e. N

o c

lea

r pa

ttern

is n

ote

d, in

clu

din

g o

ffse

t we

llsw

ith la

rge

co

ntra

st in

pa

y a

nd

stru

ctu

rally

low

we

lls w

ithh

igh

er p

ay

ca

lcu

latio

ns

. Ma

ps

of c

um

ula

tive

oil a

nd

ga

sp

rod

uc

tion

in th

e“h

igh

vo

lum

e a

rea”

sh

ow

sim

ilar

va

riatio

n o

n a

we

ll-to-w

ell le

ve

l.

1261

1205

1202

12071228

1229

1201

1206

1209

1208

Phi-BVW= hydrocarbon pore volume

additio

nal s

ectio

n is

availa

ble

for h

ydro

carb

on

accum

ula

tion.

Well #

1228 is

locate

d a

dja

ce

nt to

well #

120

7 in

a s

tructu

rally

hig

h p

ositio

non th

e to

p o

f the S

an

Andre

s, b

ut th

e p

ay in

terv

al is

aro

und 3

5 fe

et lo

wer.

The p

hi-B

VW

pro

files a

re in

sharp

contra

st to

one a

no

ther, 7

.77 (o

ne o

f the

hig

hest v

alu

es) v

s. 3

.69.A

dd

itionally, th

e m

axim

um

pay v

alu

es (p

hi-B

VW

)fo

r ind

ivid

ual p

oin

ts d

eclin

e fro

m 0

.1 to

0.5

in w

ell #

12

28, a

s in

dic

ate

d b

yth

e o

range d

ashed lin

e in

the p

hi-B

VW

dep

th p

lot. O

ther w

ells

follo

w th

istre

nd o

f phi-B

VW

declin

e w

ith d

epth

sugge

stin

g a

declin

e in

hydro

ca

rbon

satu

ratio

n, p

erh

aps a

n in

dic

atio

n o

f transitio

n.

Most o

f the in

dic

atio

ns o

f pa

y (p

hi-B

VW

), oth

er th

an in

well #

1261, re

sid

eat e

levatio

ns a

bove -7

88 fe

et.

This

may b

e a

n in

dic

atio

n o

f the p

roxim

ity o

fan o

il/wate

r co

nta

ct.

ii

PH

I-BV

WA

NA

LY

SIS

GE

NE

RA

LO

BS

ER

VA

TIO

NS

OF

PH

I-BV

W P

LO

TS

AN

D M

AP

PIN

G

Afte

r petro

physic

al c

ut-o

ffs a

re a

pplie

d a

nd th

e p

ay in

terv

als

of re

serv

oir a

re id

entifie

d, e

ffectiv

e p

oro

sity

can b

esu

btra

cte

d fro

m th

e B

VW

, the b

ulk

volu

me w

ate

r, to e

stim

ate

hydro

carb

on p

ore

volu

me

. Dis

pla

yin

g a

depth

pro

fileof p

hi-B

VW

can

pro

vid

e a

n in

dic

atio

n o

f a h

ydro

carb

on tra

nsitio

n z

one, w

here

valu

es d

ecre

ase

with

depth

,eventu

ally

dro

pp

ing to

zero

at th

e h

ydro

carb

on/w

ate

r conta

ct. S

imila

rly, wid

espre

ad s

ca

tterin

g o

f poin

ts w

ith n

opa

ttern

reveals

com

ple

x h

ete

rogeneity

with

no tra

nsitio

n z

one o

r oil o

r gas w

ate

r conta

ct.

The p

hi-B

VW

de

pth

plo

t show

s s

om

e v

ague p

atte

rns re

late

d to

local re

se

rvoir h

ete

rogen

eity

that a

ppears

to b

ede

velo

ped a

t the

well s

cale

, rela

ted to

the s

trong k

ars

t overp

rintin

g th

at h

as g

enera

lly re

duced th

e m

ore

contin

uous

pa

y d

evelo

ped in

the o

verly

ing

gra

insto

ne-p

acksto

nes.T

hu

s, k

ars

t dia

gen

esis

pays a

sig

nific

an

t role

in th

ehe

teogeneity

in th

e“h

igh v

olu

me a

rea

”.

Well-s

cale

hete

rogeneity

is s

imila

rly re

flecte

d in

the c

um

ula

tive p

roductio

n a

nd s

eis

mic

attrib

ute

data

. Seis

mic

attrib

ute

analy

sis

suggests

an e

lem

ent o

f stru

ctu

ral c

ontro

l on th

is h

ete

rog

eneity.

Low

mean im

pedance in

the re

serv

oir in

terv

al h

as

been s

how

n to

corre

spond

genera

lly to

hig

h m

ean

poro

sity. H

ow

ever, lo

wer m

ean im

pedance a

lso

appears

to c

orre

late

with

low

er c

um

ula

tive

hydro

carb

on

pore

volu

me fro

m P

hi-B

VW

, as is

show

nby w

ells

#12

61 a

nd #

1228

(whic

h h

ave a

thic

ker

kars

t zone), c

om

pare

d to

wells

#1202 a

nd #

1228

(whic

h h

ave

a th

inner k

ars

t zone).

This

corre

sponde

nce b

etw

een h

igh p

oro

sity

and lo

whydro

carb

on

pore

volu

me is

most lik

ely

expla

ined b

yth

e fa

ct th

at th

e h

igh p

oro

sity

is d

evelo

pe

d d

eeper in

the re

serv

oir in

terv

al (a

s w

as in

dic

ate

d b

y th

e c

ente

rof g

ravity

ma

p) a

nd in

are

as w

ith th

icker k

ars

t, the

low

er p

oro

sity

upper re

serv

oir w

ill be c

ut o

ut, s

o th

at

only

the d

ee

per h

igh p

oro

sity

inte

rval w

ill contrib

ute

to th

e m

ean

poro

sity.

Am

ost p

ositiv

e c

urv

atu

re m

ap (s

how

ing a

ntifo

rmbendin

g) e

xtra

cte

d fro

m th

e s

eis

mic

data

volu

me

alo

ng a

Devonia

n h

oriz

on a

ppro

xim

ate

ly 0

.6 s

econds

belo

w th

e S

an

Andre

s s

ho

ws th

at th

ere

is a

sig

nific

ant d

eep-s

eate

d s

tructu

ral c

ontro

l to th

enorth

west-tre

ndin

g fe

atu

res in

the

“hig

h v

olu

me

are

a”.

As c

an b

e s

een b

y th

e in

terle

aved

most

positiv

e c

urv

atu

re a

nd m

ea

n re

serv

oir in

terv

al

impedance m

aps, th

ere

is a

lso a

n in

dic

atio

n th

at

cro

sscuttin

g n

orth

to n

orth

east-tre

ndin

g fe

atu

res o

nth

e D

evonia

n s

urfa

ce a

lso im

pacte

d p

oro

sity

develo

pm

en

t in th

e S

an

An

dre

s.

Am

ost p

ositiv

e c

urv

atu

re m

ap e

xtra

cte

d a

long th

e“x

mark

er s

how

s s

om

e o

f the

sam

e s

tructu

ral tre

nds a

sth

e D

evonia

n h

oriz

on b

ut a

lso s

how

s a

finer n

etw

ork

of lin

eam

ents

that e

nclo

se

are

as w

ith d

iam

ete

rs o

nth

e o

rder o

f 1500 ft (4

50 m

).T

hese fe

atu

res m

ay

indic

ate

rese

rvoir c

om

partm

enta

lizatio

n a

t a s

ingle

-w

ell s

cale

.

SE

ISM

ICA

TT

RIB

UT

EA

NA

LY

SIS

Mo

st p

os

itive

vo

lum

etric

cu

rva

ture

ex

trac

ted

alo

ng

the

“x

”m

ark

er

ho

rizo

n s

up

erim

po

se

d o

n th

e m

ea

n im

pe

da

nc

e m

ap

for th

e b

as

e k

ars

t to“x

”m

ark

er in

terv

al. B

lac

k c

orre

sp

on

ds

to tig

ht p

os

itive

(an

tiform

al)

cu

rva

ture

.

Mo

st p

os

itive

vo

lum

etric

cu

rva

ture

ex

trac

ted

alo

ng

a D

ev

on

ian

ho

rizo

n(a

pp

rox

ima

tely

0.6

se

co

nd

s b

elo

w th

e S

an

An

dre

s) s

up

erim

po

se

d o

n th

em

ea

n im

pe

da

nc

e m

ap

for th

e b

as

e k

ars

t to“x

”m

ark

er in

terv

al. B

lac

kc

orre

sp

on

ds

to tig

ht p

os

itive

(an

tiform

al) c

urv

atu

re.

1207

1228

12611202

1207

1228

12611202