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Comparison of the Bouguer gravity anomaly, heat flow, depth to basement maps and seismic reflection data shows that the areas with high heat flows are associated with low negative gravity values (−10 to −25).
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From the seismic interpretation, the graben in the basin is associated with low heat flow and very low negative Bouguer gravity anomalies while the closely packed contours of the heat flow and gravity maps are attributed to the presence of faults and undulating folds.
The graben in the basin is associated with low heat flow and very low negative Bouguer gravity anomaly.
A negative gravity low of ~ 70 mgal is observed along the Andaman trench followed by a broad and distinct gravity low with an amplitude of − 100 to − 110 mgal observed over the outerarc and forearc basins.
A rigid ice shell on Saturn's largest moon Titan resists the upward pressure of a buoyant root, whose low density produces a negative gravity anomaly.
The Beppu-Shimabara Graben is characterized by steeply low-gravity anomalies and significant negative gravity anomalies in the eastern edge.
These concentrated areas of mass, referred to as mascons, usually have a positive gravity anomaly peak and surrounded by negative gravity anomalies with low geographical elevation.
The buoyancy in the mantle wedge and the low density sedimentary body possibly yield the significant negative gravity anomaly.
The Beppu Shimabara Graben shown in Fig. 1 corresponds to the negative gravity anomaly area in the north-east and to a gravity low area less than about 20 mGal in the south-west.
The low-pass filtered gravity component image (Res(m, n)) is interpreted to depict the lowest geological architecture within the study area, which reflects that there may be a pair of the NW-trending uplift zone of the mantle and/or the basement with positive gravity anomaly and the depression zone of the mantle and/or the basement with negative gravity anomaly.
Reservoir area with many production wells have negative gravity changes.
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