HiRISE stereo DTMs / Edwin Kite
Acknowledgements:
These DTMs were produced using the SOCET SET workstation at the SETI Institute, generously made available to me by Cynthia Phillips (SETI). I am also grateful to Ross Beyer (Ames/SETI), Annie Howington-Kraus (USGS), Audrie Fennema (LPL), and Sarah Mattson (LPL) for help with DTM generation.
Note on usage:
You are welcome to download and use these DTMs for any science purpose without contacting me. However, please be aware that these were generated for a particular task that did not require editing to the standards of PDS-released DTM products. In particular, I have made minimal use of Interactive Terrain Edit (ITE) for blunder removal. Informally, short wavelength slopes are more reliable than long wavelength slopes; relative elevations are more reliable than absolution elevations. For a description of other common artifacts, see the HiRISE team's DTM notes page. For Arc use, I recommend the USGS image toolbox to convert 32-bit NODATA values.
Cratered cones
Valles Marineris plateau channel networks
Aeolis-Zephyria
NW Hellas Basin ("taffy terrain")
Mojave Crater
Glacial channels
PSP_002232_2180/PSP_002377_2180 ("Cydonia1"):
PSP_002233_2225/PSP_002866_2225 ("Acidalia3"):
PSP_006858_1420/PSP_007003_1420 ("Hellas2r"):
PSP_006278_1410/PSP_010563_1410 ("Hellas4r"):
PSP_007715_1420/ESP_016022_1420 ("Hellas5"):
PSP_007781_1410/PSP_008137_1410 ("Hellas7"):
PSP_003223_1755/PSP_003724_1755 ("Juventae1"):
PSP_005161_1720/ESP_016237_1720 ("Ganges1"):
PSP_004423_1755/PSP_005412_1755 ("Juventae2"):
PSP_006683_1740/PSP_010322_1755 ("Aeolis1"):
PSP_007975_1755/PSP_009623_1755 ("Aeolis2"):
ESP_013968_1890/ESP_014390_1890 ("MojaveNE1"):
ESP_016260_2295/ESP_016339_2295 ("Lyot1"):