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GADJAH MADA GEOPHYSICS EXPLORATION GROUP
RESEARCH OBJECTIVES We are interested in Geophysical exploration, seismic profilling (reflection or refraction), though we employ all other geophysical techniques when appropriate, and also attempt to integrate geological information to compute & analyze geophysical data closely into our models. PEOPLE This Group led by Drs. Sismanto, MSi. The members are students who interested in Geophysical exploration. RESEARCH LINKAGES
RESEARCH
AVO (AMPLITUDE VARIATION WITH OFFSET) ANOMALY By: Purbo
Santoso AVO
(Amplitude Variation with Offset) anomaly is often indicates the existence
of gas accumulation, therefore it is important to look for AVO anomalies
in an exploration area. An
attempt to carry out AVO
mapping has been conducted in the Air Benakat and Gumai formation of the
Betara Deep area, Jabung block, Jambi. In order to get more detail
results, each formation was divided into three intervals, i.e. Air Benakat
A (top of Air Benakat – 80 ms under the top), Air Benakat B (between Air
Benakat A and C), and Air Benakat C (base of Air Benakat – 80 ms over
the base) for the Air Benakat formation, while the Gumai formation
consists of Gumai A (top of Gumai – 140 ms under the top),
Gumai B (between Gumai A and C), and Gumai C (base of Gumai – 140
ms over the base). AVO mapping was conducted in these
intervals by using data of P*G attribute as a result of AVO
processing of the Betara Deep’s seismic data. Most
of distribution of AVO anomalies in the Air Benakat formation was found in
Air Benakat B, Air Benakat A had less anomalies than Air Benakat B, and
the least distribution was in Air Benakat C. In the Gumai formation, Gumai
A had more AVO anomalies than Gumai B, whereas Gumai C had no anomalies at
all. In overall, more AVO anomalies were found in the Air Benakat formation than that found in the Gumai formation, and AVO anomalies in both formations can be found in the southern part of the Betara Deep where there were a lot of fault structures that may be considered as hydrocarbon trap.
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