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.
| Traverse Ramp in East Coprates Chasma: ESP_076818_1640 ESP_076752_1640 (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 | -15.6 | 306. | 9.47 | 23.67 | 38.7 | 36.8 |
| Lobate Gully Debris Apron: ESP_076771_1445 ESP_076138_1445 (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 | -35.3 | 152. | 4.56 | -20.2 | 47.9 | 41.2 |
| Downwind Hellespontus Regional Barchan Dunes: ESP_076841_1380 ESP_076221_1380 (Interval in Earth days: 48) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -41.4 | 44.5 | -10. | 12.82 | 53.9 | 43.1 |
| Gully Monitoring and Topography: ESP_076981_1420 ESP_085750_1420 (Interval in Earth days: 683) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.6 | 182. | -1.8 | -24.5 | 53.1 | 53.6 |
| Aurorae Chaos: ESP_077002_1705 ESP_077068_1705 (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 | -9.55 | 325. | -3.8 | -17.7 | 39.8 | 41.6 |
| Valley South of Ares Vallis: ESP_076896_1890 ESP_076962_1890 (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 | 9.103 | 335. | 8.83 | -5.66 | 37.4 | 38.6 |
| Gullies on Massif in Argyre Region: ESP_076923_1345 ESP_076224_1345 (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 | -45.0 | 325. | 7.99 | -7.78 | 56.6 | 46.5 |
| Candidate Mud Volcanoes Targeted by Zhurong Rover: ESP_076891_2050 ESP_077023_2050 (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 | 24.74 | 109. | 5.44 | -19.3 | 43.1 | 44.2 |
| Terrain Sample in Claritas Fossae: ESP_076767_1510 ESP_076833_1510 (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 | -28.5 | 260. | 10.3 | -4.76 | 43.7 | 45.6 |
| Landforms in Utopia Planitia: ESP_077063_2110 ESP_077274_2110 (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 | 30.56 | 95.9 | -5.2 | 13.64 | 45.5 | 42.9 |
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