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.
Inner Channel Deposit in Kasei Vallis: PSP_007825_2010 ESP_035463_2010 (Interval in Earth days: 2153) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 20.84 | 287. | -3.9 | 12.13 | 41.7 | 43.8 |
Potential Fan Deposit in Ritchey Crater with Clays: PSP_007363_1510 PSP_008365_1510 (Interval in Earth days: 78) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -28.4 | 308. | 3.89 | -7.30 | 59.7 | 71.0 |
Distal Rampart of Crater in Isidis Region: PSP_007740_1920 ESP_016047_1920 (Interval in Earth days: 647) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 12.01 | 89.5 | -2.3 | 18.67 | 43.2 | 38.0 |
Crater in the Adamas Labyrinthus Region Seen in THEMIS Image V21701005: PSP_007713_2170 PSP_009862_2170 (Interval in Earth days: 167) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.45 | 103. | -4.4 | 10.64 | 41.9 | 45.6 |
Distal End of Lethe Vallis: PSP_007263_1845 PSP_007553_1845 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.500 | 156. | -7.8 | 5.828 | 42.2 | 43.6 |
Fresh Rayed Crater: PSP_007707_1600 ESP_071927_1600 (Interval in Earth days: 5003) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -19.5 | 274. | -2.6 | 15.67 | 58.5 | 65.0 |
Knobs and Cones in Acidalia Planitia: PSP_007506_2220 ESP_051759_2220 (Interval in Earth days: 3448) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 41.57 | 354. | 3.16 | 20.33 | 43.2 | 38.9 |
Wall Layers of Tooting Crater: PSP_007907_2035 ESP_019115_2035 (Interval in Earth days: 873) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.18 | 208. | -2.3 | 5.434 | 41.6 | 48.0 |
Western Rim and Ejecta of Mojave Crater: PSP_007494_1875 PSP_007850_1875 (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 | 7.410 | 326. | 8.05 | -4.28 | 42.0 | 45.7 |
Upper Section of Northern Olympus Mons Basal Scarp: PSP_007445_2035 PSP_008447_2035 (Interval in Earth days: 78) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 22.90 | 223. | -1.4 | -13.8 | 40.1 | 44.4 |
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