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.
Light-Toned Layering in Ius Chasma: PSP_005940_1710 ESP_013627_1710 (Interval in Earth days: 599) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.73 | 280. | -8.5 | 4.624 | 34.3 | 39.6 |
Unnamed Well-Preserved Crater: PSP_006837_1345 PSP_007127_1345 (Interval in Earth days: 22) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -45.1 | 274. | -4.9 | 13.74 | 63.8 | 67.5 |
Central Peak of Well-Preserved Unnamed Crater: PSP_006782_1630 PSP_006927_1630 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -16.7 | 331. | -6.1 | 5.697 | 45.0 | 46.2 |
Valley-Like Forms Seen in MOC Images: PSP_006942_1690 PSP_010871_1690 (Interval in Earth days: 306) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -10.7 | 282. | -6.0 | 17.07 | 44.2 | 58.2 |
Primary Cavity of Rayed Gratteri Crater: PSP_005732_1620 ESP_011507_1620 (Interval in Earth days: 450) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -17.7 | 200. | -2.5 | 11.09 | 33.6 | 57.9 |
Bright Gully Deposits in A Fresh Impact Crater: PSP_006922_2120 PSP_007067_2120 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 31.87 | 102. | 1.45 | 11.11 | 42.0 | 40.7 |
Giza Region Unfrosted: PSP_004736_0950 PSP_005119_0950 (Interval in Earth days: 30) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -84.8 | 65.7 | 1.48 | -14.5 | 64.0 | 68.7 |
Gullies with Bright Color Deposits: PSP_005082_1365 ESP_012703_1365 (Interval in Earth days: 594) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -43.0 | 309. | -0.9 | 23.99 | 38.4 | 46.0 |
Hanging Valley in Minio Vallis: PSP_006470_1760 PSP_007762_1760 (Interval in Earth days: 101) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.14 | 208. | 0 | 23.15 | 36.5 | 48.2 |
Contact between Polygon and Massif: PSP_005700_2200 ESP_011818_2200 (Interval in Earth days: 477) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 39.77 | 346. | 0 | -24.3 | 59.2 | 72.7 |
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