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Seismoacoustic Study of the Shallow Gas Transport and ... - E-LIB

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Chapter 2<br />

reflections. These transparent seismic reflections represent mud flows deposited during<br />

eruptive episodes. Therefore, three mud chambers represent three periods <strong>of</strong> intense<br />

eruptive activity.<br />

Figure 10 Structural <strong>and</strong> evolutionary <strong>of</strong> <strong>the</strong> MSU mud volcano. Red patches indicate <strong>the</strong> gas/gas hydrate<br />

reservoirs. Dark green arrows show <strong>the</strong> gas/fluid migration pathways. Light green arrows show <strong>the</strong> gas may<br />

derive from <strong>the</strong> shallow subsurface. Dotted lines indicate <strong>the</strong> downward bending <strong>of</strong> sediment layers in <strong>the</strong><br />

feeder channel, which can be traced towards <strong>the</strong> undisturbed sedimentary strata. Two mud chambers <strong>and</strong> a<br />

small chamber are included. Faults are indicated <strong>the</strong> vertical black lines.<br />

Feeder channels <strong>of</strong> mud volcanoes are interpreted in six locations as <strong>the</strong> main<br />

pathways for gas <strong>and</strong> fluid upward migration. Main characteristics are a flat top, wide<br />

mud chambers <strong>and</strong> wide feeder channels, which indicate low mud viscosity, transport <strong>of</strong><br />

large gas <strong>and</strong> mud volume <strong>and</strong> long lasting activity, similar to <strong>the</strong> evidence provided by<br />

Somoza et al. (2012). Downward bending <strong>of</strong> reflections at <strong>the</strong> base <strong>of</strong> mud chambers<br />

reveals a significant collapse due to a volume loss <strong>and</strong> depressurization associated with<br />

mud eruptions. On <strong>the</strong> flanks <strong>of</strong> <strong>the</strong> feeder channel, bright spots <strong>and</strong> blurred margins<br />

indicate <strong>the</strong> lateral transport <strong>of</strong> gas into <strong>the</strong> surrounding high permeable (s<strong>and</strong>y) sediment<br />

layers. This may originate from free gas transported with <strong>the</strong> mud, but also from gas<br />

hydrate decomposition in case that <strong>the</strong> mud eruption provides fast vertical heat transport.<br />

Isotopic analysis showed that <strong>the</strong> gas is <strong>of</strong> mixed biogenic <strong>and</strong> <strong>the</strong>rmogenic origin<br />

(Ivanov et al., 1996; Limonov et al., 1997). The biogenic gas may derive from <strong>the</strong><br />

shallow subsurface, which is rich in <strong>the</strong> terrigenous organic matter from <strong>the</strong> Danube <strong>and</strong><br />

Dniepr rivers (Limonov et al., 1997). Particularly <strong>the</strong> <strong>the</strong>rmogenic gas migrates upward<br />

64

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