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.
Wrinkle Ridge Cross-Cutting Relationships in Hesperia Planum : PSP_002544_1540 PSP_002689_1540 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -25.8 | 116. | 2.57 | 16.59 | 59.9 | 57.6 |
Low-Latitude North Polar Layered Deposits and Basal Unit Contact: PSP_001548_2755 PSP_001694_2755 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 84.4 | 142. | 1.30 | 17.73 | 75.0 | 74.8 |
Boulder Tracks with Boulders at Ends: PSP_001730_1740 PSP_002086_1740 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.87 | 16.4 | -2.4 | 21.5 | 57.0 | 54.7 |
Fresh-Looking Gullies: PSP_001714_2390 PSP_001846_2390 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 58.73 | 82.3 | 3.50 | -8.24 | 57.8 | 60.7 |
Exposure of Polar Layered Deposits Not Well Covered by Mars Global Surveyor: PSP_001342_2680 PSP_001568_2680 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 88.04 | 62.4 | -6.0 | -13.1 | 70.2 | 72.6 |
Ganges Mensa : PSP_002550_1725 PSP_003618_1725 (Interval in Earth days: 83) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.25 | 311. | -4.4 | 26.16 | 56.4 | 49.8 |
White Rock Deposits: PSP_002033_1720 PSP_002099_1720 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.01 | 25.0 | 5.96 | -17.5 | 56.7 | 58.4 |
Exhumed Faults in Huo Hsing Vallis: PSP_001596_2080 PSP_002216_2080 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 27.71 | 67.3 | -0.7 | -24.8 | 49.5 | 57.7 |
Gamboa Crater Central Uplift in Acidalia Planitia : PSP_002721_2210 ESP_028724_2210 (Interval in Earth days: 2026) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.77 | 315. | 0.64 | -12.1 | 66.1 | 59.9 |
Circular Light-Toned Layering in Candor Chasma: PSP_002076_1735 PSP_002498_1735 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.23 | 290. | 5.75 | -6.89 | 56.1 | 56.6 |
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