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.
| Gullies in Crater in Terra Cimmeria : ESP_056923_1330 ESP_057899_1330 (Interval in Earth days: 76) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -46.4 | 154. | -4.3 | 17.05 | 43.9 | 36.5 |
| Central Pit of Asimov Crater : ESP_057034_1330 ESP_057245_1330 (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 | -46.8 | 4.83 | -5.7 | 3.292 | 42.8 | 39.8 |
| Fresh Crater and Landslide : ESP_056990_1530 ESP_057412_1530 (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 | -26.5 | 122. | 0 | 24.05 | 40.2 | 33.1 |
| Tantalus Fossae : ESP_056721_2190 ESP_057275_2190 (Interval in Earth days: 43) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 38.54 | 255. | 3.34 | -9.01 | 73.3 | 73.1 |
| Hunt for Small Ancient Impact Craters near Nili Fossae: ESP_057018_2015 ESP_057229_2015 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.18 | 72.5 | -7.4 | 3.427 | 61.6 | 59.7 |
| Small Valleys in Southern Highlands: ESP_056967_1480 ESP_057178_1480 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -31.8 | 31.1 | -5.5 | 4.442 | 40.8 | 37.4 |
| Navua Valles : ESP_056952_1440 ESP_057163_1440 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -35.8 | 81.3 | -6.8 | 2.199 | 41.5 | 38.1 |
| Northern Mid-Latitude Crater Floor Features : ESP_056994_2150 ESP_083910_2150 (Interval in Earth days: 2097) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 34.48 | 5.21 | 0 | 18.53 | 70.8 | 70.0 |
| Light-Toned Layered Deposits in Argentea Planum : ESP_056733_1060 ESP_056746_1060 (Interval in Earth days: 1) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -74.0 | 306. | 8.34 | 25.36 | 59.0 | 57.6 |
| Cratered Features in Olympus Mons Aureole : ESP_057052_2145 ESP_057131_2145 (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 | 34.27 | 225. | -29. | 3.024 | 72.2 | 70.0 |
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