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 in Tempe Terra: ESP_036412_2175 ESP_037968_2170 (Interval in Earth days: 122) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 37.02 | 300. | -3.4 | -4.37 | 47.1 | 65.5 |
| Chasma Boreale North Margin Scarp: ESP_036515_2650 ESP_037056_2650 (Interval in Earth days: 42) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 85.01 | 342. | -6.8 | -15.8 | 66.4 | 74.0 |
| Candidate 2020 Mission Landing Site in Gusev Crater: ESP_036720_1655 ESP_042707_1655 (Interval in Earth days: 467) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.5 | 175. | 12.6 | 0.042 | 61.2 | 51.3 |
| Crater Exposing Bedrock: ESP_036448_1710 ESP_062927_1715 (Interval in Earth days: 2063) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.97 | 42.4 | 6.12 | -3.07 | 59.3 | 59.2 |
| Small Crater on North Polar Layered Deposits: ESP_036498_2630 ESP_036458_2630 (Interval in Earth days: 3) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 83.00 | 94.8 | -8.4 | 5.862 | 65.0 | 63.8 |
| Candidate ExoMars Landing Site at Coogoon Valles: ESP_036714_1975 ESP_037426_1975 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.18 | 337. | -5.3 | 6.643 | 50.7 | 54.3 |
| Light-Toned Layered Deposits at Terminus of Ladon Valles: ESP_036543_1595 ESP_037110_1595 (Interval in Earth days: 45) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -20.2 | 329. | 6.72 | -5.81 | 65.4 | 63.8 |
| Layered Terrain and Crater Ejecta Deposits in Arabia Terra: ESP_036541_1945 ESP_037609_1945 (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 | 14.54 | 21.3 | -6.1 | 14.01 | 50.6 | 54.9 |
| Eroded Terrain in Aeolis Region: ESP_036589_1725 ESP_037789_1725 (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 | -7.45 | 152. | 8.82 | -7.46 | 58.1 | 57.8 |
| Steepest North Polar Scarp: ESP_036506_2640 ESP_036546_2640 (Interval in Earth days: 3) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 83.87 | 235. | -10. | -22.4 | 65.7 | 67.0 |
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