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Figure 3 - GRABEN SYSTEMS (DYKE SWARMS) OF THE MBOKOMU MONS REGION, ALONG PARGA CHASMATA, 2400 KM SE OF ATLA REGIO, VENUS.

Figure 3: A) Magellan SAR left look image of Cycle 1. B) Extensional lineaments; 6,650 mapped so far at 1:500,000 scale. Grouped into graben sets based on trend and geometry. C) Generalized mapping of grabens in the vicinity of Mbokomu Mons superimposed on SAR image. Stars locate multiple centres of radiating graben systems associated Mbokomu Mons. Note presence of circumferential set associated (purple) indicating a corona-like character associated with this Mons [9]. Number of additional linear and circumferential sets are present (see discussion in text). D) Lava flows and shield volcanoes.
A) Magellan SAR left look image of Cycle 1. B) Extensional lineaments; 6,650 mapped so far at 1:500,000 scale. Grouped into graben sets based on trend and geometry. C) Generalized mapping of grabens in the vicinity of Mbokomu Mons superimposed on SAR image. Stars locate multiple centres of radiating graben systems associated Mbokomu Mons. Note presence of circumferential set associated (purple) indicating a corona-like character associated with this Mons [9]. Number of additional linear and circumferential sets are present (see discussion in text). D) Lava flows and shield volcanoes.
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