Planned stereo pairs have suitable stereo convergence angles and illumination by design.
In addition to planned stereo pairs, the Pairendipity software can identify overlapping
HiRISE images that are serendipitously suitable for stereo processing and find stereo
pairs within the CTX dataset.
Planned HiRISE stereo pairs are listed in the “Stereo Pair List (CSV)” link below.
Since this list is based on produced stereo anaglyphs it also contains a few serendipitous
pairs that underwent special processing. Most serendipitous HiRISE stereo pairs are listed
in the “Pairendipity Stereo” link, while CTX stereo pairs are listed
in “Pairendipity CTX Stereo”.
Images taken close together in time minimize illumination and frost differences and are
especially useful (see the Delta-Days column in the Pairendipity files or difference
the orbit numbers in the image IDs in the Stereo Pair List file). Stereo pairs
with both images planned within the same 14-day (168-orbit) operations cycle are known as SPORCs.
Finely-Layered Deposits in Henry Crater: PSP_008072_1905 PSP_009153_1905 (Interval in Earth days: 84) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 10.17 | 24.0 | 0.27 | 15.57 | 45.7 | 48.8 |
Hematite in West Candor Chasma: PSP_007601_1745 PSP_010449_1745 (Interval in Earth days: 222) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.55 | 286. | 7.08 | -20.0 | 48.5 | 59.7 |
Interaction between Unnamed Crater Ejecta and Pre-Exsisting Terrain: PSP_007681_2000 PSP_008406_2000 (Interval in Earth days: 57) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 19.66 | 259. | -6.6 | 23.65 | 41.5 | 41.9 |
Central Peak and South Rim of Large Fresh Crater in Isidis Basin: PSP_007107_1900 PSP_009823_1900 (Interval in Earth days: 211) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 10.02 | 94.3 | 0.07 | -12.8 | 39.2 | 52.4 |
Fresh 7-Kilometer Diameter Crater with Bright Rayed Ejecta: PSP_007731_2060 ESP_026310_2060 (Interval in Earth days: 1448) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 25.77 | 333. | 1.95 | 28.52 | 40.6 | 38.7 |
Well-Preserved 15-Kilometer Diameter Crater Near Nili Fossae: PSP_007912_2030 ESP_018342_2030 (Interval in Earth days: 813) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 22.63 | 71.3 | 0.11 | 15.86 | 41.5 | 43.9 |
Crater with Multiple Gully Orientations: PSP_007001_2200 PSP_007937_2200 (Interval in Earth days: 73) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 39.48 | 105. | -8.6 | 6.751 | 45.7 | 41.3 |
Hellas Planitia: PSP_007781_1410 PSP_008137_1410 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.4 | 55.7 | 6.07 | -3.19 | 72.0 | 76.2 |
Gullies as Seen in MOC Image M02-02681: PSP_007213_1400 ESP_042618_1400 (Interval in Earth days: 2759) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.6 | 86.3 | 2.71 | 26.46 | 65.4 | 65.6 |
Fractured Terrain in Elysium Planitia: PSP_007711_1870 PSP_008067_1870 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 6.775 | 161. | 7.20 | -4.18 | 43.9 | 47.3 |
Page 769 of 851 (8,502 images) |