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Abalos Undae dunes at Abalos Scopuli, the scarp of Abalos Mensa. The ice layers on the cap and basal formations are also visible. The picture was take
Abalos Undae dunes at Abalos Scopuli, the scarp of Abalos Mensa. The ice layers on the cap and basal formations are also visible. The picture was taken by the HiRISE camera on board the Mars Reconnaissance Orbiter and was enhanced by NASA in RGB colour.
Abalos Undae at Abalos Scopuli, the scarp of Abalos Mensa
Abalos Undae at Abalos Scopuli, the scarp of Abalos Mensa
Dunes in Abalos Undae. The blue areas indicate the presence of dunes of basaltic origin, while the light-colour areas are probably dust.
Dunes in Abalos Undae. The blue areas indicate the presence of dunes of basaltic origin, while the light-colour areas are probably dust.
Gypsum deposits in the dunes of Abalos Undae
Gypsum deposits in the dunes of Abalos Undae
Hyperboreae Undae dunes shown with surface frost. The dunes become darker when the frost sublimates from solar heating and the dark sands are revealed
Hyperboreae Undae dunes shown with surface frost. The dunes become darker when the frost sublimates from solar heating and the dark sands are revealed.
Coexistence of linear and barchan forms at Hyperboreae Undae. A study has been undertaken to explain the coexistence of these two forms. The location
Coexistence of linear and barchan forms at Hyperboreae Undae. A study has been undertaken to explain the coexistence of these two forms. The location of the initial study site is at the boundary of Hyperboreae Undae with Boreum Cavus.
Hyperboreae Undae barchanoid and linear dunes from NASA's Thermal Emission Imaging System (THEMIS)
Hyperboreae Undae barchanoid and linear dunes from NASA's Thermal Emission Imaging System (THEMIS)
Hyperboreae Undae from NASA's Thermal Emission Imaging System (THEMIS)
Hyperboreae Undae from NASA's Thermal Emission Imaging System (THEMIS)