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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)
The Hagal dune field. Image was taken on 6 February 2016 at 15:16 local Mars time.
The Hagal dune field. Image was taken on 6 February 2016 at 15:16 local Mars time.
Detail of the dots and dashes of the dunes on 6 February 2016, at 15:16 local Mars time.
Detail of the dots and dashes of the dunes on 6 February 2016, at 15:16 local Mars time.
Detail of the dots and dashes of the dunes with distance scale
Detail of the dots and dashes of the dunes with distance scale