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.
Crater with Two Concentric Central Stuctures: ESP_018282_1640 ESP_019271_1640 (Interval in Earth days: 77) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.8 | 275. | 5.65 | -11.2 | 63.6 | 61.9 |
Streamlined Form at the Confluence of Tiu Valles and Ares Vallis: ESP_018491_1975 ESP_018636_1975 (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 | 17.23 | 326. | -4.3 | 11.33 | 47.5 | 46.6 |
Exposure of North Polar Layered Deposits in Area Not Well Observed: ESP_018376_2685 ESP_019113_2685 (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 | 88.32 | 200. | -20. | -13.4 | 65.1 | 71.7 |
Kasei Valles North Wall Terraces: ESP_018149_2060 ESP_018439_2060 (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 | 25.94 | 302. | -8.0 | 18.69 | 44.6 | 43.2 |
Dark Outcrop: ESP_018292_1780 ESP_019492_1780 (Interval in Earth days: 94) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.92 | 0.09 | 11.0 | -12.0 | 54.7 | 55.9 |
Two Distinct Surfaces along Mesa Wall in Deuteronilus Mensae: ESP_018225_2275 ESP_018146_2275 (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 | 47.18 | 22.7 | 5.82 | -17.3 | 43.5 | 45.3 |
Possible MSL Rover Landing Site in Gale Crater Covering North Central Mound: ESP_018287_1755 ESP_018788_1755 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.58 | 137. | -0.4 | 23.35 | 57.0 | 54.9 |
Bull's-Eye Impact Crater: ESP_018522_2270 ESP_019010_2270 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 46.56 | 194. | 2.26 | -21.5 | 45.4 | 51.7 |
Future Mars Landing Site in Acidalia Mensa: ESP_018161_2270 ESP_018227_2270 (Interval in Earth days: 5) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 46.68 | 331. | -1.6 | -15.5 | 43.8 | 45.4 |
Future Mars Landing Site in Antoniadi Crater: ESP_018105_2045 ESP_018250_2045 (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 | 24.05 | 63.0 | -0.2 | 13.32 | 44.2 | 43.5 |
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