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.
Central Pit Gullies in Asimov Crater: ESP_013123_1330 ESP_013268_1330 (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 | -46.8 | 4.93 | 13.8 | 22.63 | 42.3 | 40.3 |
Phyllosilicate Diversity North of Mawrth Vallis: ESP_013150_2070 ESP_014139_2070 (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 | 26.60 | 340. | -8.4 | -22.7 | 66.9 | 56.2 |
Rocky Deposit on Crater Floor with Thermal Signature: ESP_012788_1365 ESP_013856_1365 (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 | -43.2 | 151. | 2.54 | 20.66 | 46.5 | 37.4 |
Layered Sinuous Ridge in Argyre Planitia: ESP_012848_1235 ESP_012782_1235 (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 | -56.2 | 316. | -7.0 | 6.567 | 50.2 | 50.1 |
Graben Wall with Gullies: ESP_013736_1415 ESP_013947_1415 (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 | -38.1 | 188. | 1.89 | -6.61 | 36.9 | 37.5 |
Well-Preserved Gullied Impact Crater: ESP_012925_1220 ESP_013202_1220 (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 | -57.6 | 13.0 | 7.46 | -9.50 | 48.8 | 47.4 |
Terby Crater Surroundings: ESP_013885_1520 ESP_020465_1520 (Interval in Earth days: 513) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.9 | 79.1 | 4.84 | -7.13 | 34.3 | 58.0 |
Kaiser Crater Dunes with Channels: ESP_013083_1325 ESP_013017_1325 (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 | -47.2 | 19.4 | -8.1 | 8.076 | 44.5 | 44.0 |
Gullies and Lobate Material in a Crater in the Nereidum Montes: ESP_014127_1420 ESP_020786_1420 (Interval in Earth days: 519) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.5 | 314. | -2.1 | 19.93 | 37.6 | 54.3 |
Gullies: ESP_014013_1265 ESP_014303_1265 (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 | -53.3 | 188. | 3.52 | 24.32 | 44.8 | 46.5 |
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