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Fig .1  Mars Global Surveyor (MGS) Mosaic of Ius Chasma showing branched valleys and linearly arranged pits in south and north of Ius Chasma, respectively
Fig. 2. HiRISE subset image south of Ius chasma have 1a) Steep theatre shaped headwalls 1b) short, stubby tributaries joining long main valley 1c) V-shaped valleys
Fig. 3 A profile traversing the channel (elevation data) shows that the valleys forming U shaped (X-X1) and V shaped (Y-Y1)
Fig. 5 HiRISE image having conical depressions Pits joining together in arrows. Aeolian ripples can been observed in floor

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