The Leading Edge; September 2002; v. 21; no. 9;
p. 902-905; DOI: 10.1190/1.1508955
© 2002 Society of Exploration Geophysicists
Applying 3D seismic in a complex mountainous area of Tarim Basin
Zhang Shaohua,
Yan Feng,
Li Peiming,
Li Zhenhua and
Liu Xinwen
Bureau of Geophysical Prospecting, CNPC, China
Corresponding author: lishao@public.zz.ha.cn
| The first 20% of the full text of this article appears below.
|
Complex surface and subsurface conditions in China's northern Tarim Basin make it impossible to record good 3D seismic data with conventional acquisition geometry. In addition, the thickness of the low-velocity layer varies from 3 to 150 m, making 3D static corrections a challenge.
To determine how to successfully record 3D data despite these obstacles, the Bureau of Geophysical Prospecting conducted a survey that combined regular and irregular acquisition geometry. For 3D static corrections, we carefully selected a control point for near-surface investigation, paid particular attention to the lithologic boundaries, and established an accurate near-surface model with the help of satellite data.
In an effort to evaluate oil and gas reserves of the KeLa 2 gas field in Tarim Basin, BGP geophysicists chose the Dina area as the testing ground. Structures in the Dina area are more complex than in the KeLa 2 gas field on the surface, near surface, and subsurface. Mountains, piedmont pluvial facies, and desert areas are present. Topography is rough and changes in the low-velocity zone can be dramatic both vertically and laterally (Figure 1).
View larger version (97K):
[in this window]
[in a new window]
|
Figure 1. Satellite data (a) and thickness of low velocity zone (b).
|
|
 |
3D geometry design and performance
|
|---|
Nearly a third of the northern study area is covered by gullies, bluffs, and abruptly outcropping stuctures. As a result, many shots and receivers cannot be properly positioned in a regular 3D acquisition grid. On the other hand, using only an irregular recording geometry would make it very hard to . . . [Full Text of this Article]
Copyright © 2009 by Society of Exploration Geophysicists