Title: Anticipated seismic response of reservoir sands in the Bossier Formation Upper Jurassic, Anderson co
1Anticipated seismic response of reservoir sands
in the Bossier Formation (Upper Jurassic),
Anderson county, East Texas.
- Diego Alexander Valentin,
- Robert H. Tatham and Ron Harris.
2Overview
- Introduction
- 1.1 Location and Generalities
- Problem
- Stratigraphy
- Dataset
- Methodology
- Where we are?
- What will be done?
31. Introduction
41.1 Location and Generalities
- The Tennessee Colony field is located in The
Anderson County (East Texas). - Regionally this field is located in the central
part of the East Texas basin (Klein G.D., et al
2002). - This Basin is limited to the east by the Sabine
Uplift, to the south by the Angelina Flexure zone
and to the West by the Mexia Fault zone
(Williams, R. A. et al., 2001).
Sabine Uplift
Mexia Fault zone
Anderson county
Mount Enterprise fault zone
Angelina flexure zone
Modified from Williams, R. A. et al., 2001.
51.1 Location and Generalties
- The Tennessee Colony field is composed of 11
wells from which only 7 are currently producing
dry gas. - The reservoir sands are located in the middle
part of the Bossier Formation (Upper Jurassic).
6Overview
- Introduction
- 1.1 Location and Generalities
- Problem
- Stratigraphy
- Dataset
- Methodology
- Where we are
- What will be done
72. Problem
- Uncertainty in thickness and lateral distribution
of the reservoir sand. - Small acoustic impedance contrast between the
reservoir sandstones and the encasing shales. - Conventional seismic not enough to predict sand
distribution
Pettet
Cotton Valley
Bossier
CVLM
8 Acoustic impedance vs Poissons ratio for
Bossier Formation Well Gregory A-1
9Well Gregory A-1 16200-17600ft MD
Bonner Density 2.67g/cm3 Vp4400m/s Vs2605ms
York Ss Density 2.51g/cm3 Vp4709m/s Vs3008m/s
16400
Lower Bossier Shale Density 2.66g/cm3 Vp3750m/s
Vs2297m/s
17000
17400
10 Amount of energy for the Rpp reflected wave at
the Bonner - York interface, well Gregory A-1
Bonner Density 2.67g/cm3 Vp4400m/s Vs2605ms
York ss Density 2.51g/cm3 Vp4709m/s Vs3008m/s
11Amount of energy of Rps reflected mode converted
waves at the Bonner - York interface, well
Gregory A-1
Bonner Density 2.67g/cm3 Vp4400m/s Vs2605ms
York ss Density 2.51g/cm3 Vp4709m/s Vs3008m/s
12Amount of energy of Rss(V) reflected mode
converted waves at the Bonner - York interface,
well Gregory A-1
Bonner Density 2.67g/cm3 Vp4400m/s Vs2605ms
York ss Density 2.51g/cm3 Vp4709m/s Vs3008m/s
13Amount of energy of Rss(H) reflected mode
converted waves at the Bonner - York interface,
well Gregory A-1
Bonner Density 2.67g/cm3 Vp4400m/s Vs2605ms
York ss Density 2.51g/cm3 Vp4709m/s Vs3008m/s
14 Amount of energy of Rsp reflected mode converted
waves at the Bonner - York interface, well
Gregory A-1
Bonner Density 2.67g/cm3 Vp4400m/s Vs2605ms
York ss Density 2.51g/cm3 Vp4709m/s Vs3008m/s
15Amount of energy of Rpp reflected waves at the
base of Yorks Sand interface Well Gregory A-1
York ss Density 2.51g/cm3 Vp4709m/s Vs3008m/s
Lower Bossier Shale Density 2.66g/cm3 Vp3750m/s
Vs2297m/s
16 Amount of energy of Rps reflected waves at the
base of Yorks Sand interface well Gregory A-1
York ss Density 2.51g/cm3 Vp4709m/s Vs3008m/s
Lower Bossier Shale Density 2.66g/cm3 Vp3750m/s
Vs2297m/s
17 Amount of energy of Rss(V) reflected waves at
the base of Yorks Sand interface well Gregory A-1
York ss Density 2.51g/cm3 Vp4709m/s Vs3008m/s
Lower Bossier Shale Density 2.66g/cm3 Vp3750m/s
Vs2297m/s
18 Amount of energy of Rss(H) reflected waves at
the base of Yorks Sand interface well Gregory A-1
York ss Density 2.51g/cm3 Vp4709m/s Vs3008m/s
Lower Bossier Shale Density 2.66g/cm3 Vp3750m/s
Vs2297m/s
19 Amount of energy of Rsp reflected waves at the
base of Yorks Sand interface well Gregory A-1
York ss Density 2.51g/cm3 Vp4709m/s Vs3008m/s
Lower Bossier Shale Density 2.66g/cm3 Vp3750m/s
Vs2297m/s
20Overview
- Introduction
- 1.1 Location and Generalities
- Problem
- Stratigraphy
- Dataset
- Methodology
- Where we are
- What will be done
213. Stratigraphy
- The Cotton Valley Sandstone and limestone and
Bossier Shale Formations are parts of what is
Known as Cotton Valley Group, mostly Tithonian
-Berriasian (Upper Jurassic-Lower Cretaceous).
Williams, R. A. et al., 2001.
Modified from Williams, R. A. et al., 2001.
22Bossier Formation Sequence Stratigraphic model
Cotton Valley Ss
SB3
PGC
LST
SB2
Upper Bossier
PGC
MFS
TST
SB1
Lower Bossier
LST
Modified from Klein and Chaivre, 2002.
23Sequence Stratigraphy
- The Bossier Formation can be divided in two
sequences - The first one is limited between the SB1
(CVL-Bossier contact), and SB2 (intra Bossier
boundary) was deposited during a TST. - The upper sequence between the SB2 and SB3 is
mainly a LST Prograding complex sequence caused
by a drop in the sea level caused by a climatic
change (Klein and Chaivre, 2002, Williams et al
2001).
24Depositional systems map of the Upper Bossier Fm.
Anderson
Modified from Klein and Chaivre, 2002.
25Overview
- Introduction
- 1.1 Location and Generalities
- Problem
- Stratigraphy
- Dataset
- Methodology
- Where we are
- What will be done
264. Dataset
- Well logs
- Gregory A-1, Gregory A-2, Gregory A-3, Royall
A-1, Royall A-2, Royall C-1, TDC A-1, Toole A-1. - Dipole logs Gregory A-1.
- VSP data
- Near offset pp wave well Gregory A-3.
- Near offset ss wave well Gregory A-3.
- Far offset pp and mode converted ps wave well
Gregory A-3. - Core information.
- 3D-3C seismic.
-
27Overview
- Introduction
- 1.1 Location and Generalities
- Problem
- Stratigraphy
- Dataset
- Methodology
- Where we are
- What will be done
28Methodology for the seismic Characterization of
the Bossier Formation
Available Data Checking
Literature review
Data Loading
Vsp fundamntals and understanding of the
stratigraphy and sedimentary basin evolution of
the Upper Jurasic of the East Texas Basin
Interpretation of the VSP data of the interest
horizon and well log evaluation
Understanding of the stratigraphic model for the
Bossier formation
AVO analysis of the different VSP available
surveys
Seismic Characterization of the Bossier Upper and
Lower units and correlation with well data
Test of the results in the Donatello 3D-3C seismic
29Overview
- Introduction
- 1.1 Location and Generalities
- Problem
- Stratigraphy
- Dataset
- Methodology
- Where we are?
- What will be done?
306.Where we are?
- Data was received at the end of 2008.
- Data loading and QC.
- Literature review of VSP fundamentals, Bossier
Fm., tight gas analogues and stratigraphy of the
East Texas basin. - Well correlations and log interpretation of the
available data. -
31Correlation between the Zpp (zero offset),
corridor and the synthetic log well Gregory A-3
Travis Peak
CV Sand
Bossier
York
32Correlation between the Zpp corridor and the far
offset pp VSP, well Gregory A-3.
Travis Peak
CV Sand
Bossier
Bonner
York
33Overview
- Introduction
- 1.1 Location and Generalities
- Problem
- Stratigraphy
- Dataset
- Methodology
- Where we are?
- What will be done?
347. Work Plan
- Once the data had been loaded properly, the plan
is to start interpreting the Bossier Formation
units and other horizons in the processed VSP
data. - AVO analysis.
- Integration of the well core data and the
stratigraphic model of the units to make a valid
seismic characterization. - Testing the characterization in the Donatello
3D-3C survey in order to give validity to the
model. -
35 36Acknowledgments
- Robert H. Tatham UT at Austin
- Ron Harris Anadarko
- Thomas Hess UT at Austin
-