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.
| Collapse Features on Hrad Vallis Mudflow: ESP_016467_2155 ESP_016533_2155 (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 | 35.13 | 141. | 0.42 | -15.9 | 41.1 | 42.4 |
| Layered Walls of Impact Crater in Mawrth Vallis Outcrops: ESP_016895_2045 ESP_017040_2045 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.95 | 339. | -3.5 | 8.322 | 41.6 | 41.0 |
| Source Region for Branch of Auqakuh Vallis: ESP_016826_2080 ESP_016971_2080 (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 | 27.47 | 62.7 | -7.7 | 5.246 | 41.4 | 40.6 |
| Small Volcano in Northern Syria Planum: ESP_016318_1710 ESP_016951_1710 (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 | -8.76 | 254. | 6.70 | -9.92 | 48.9 | 55.9 |
| Large-Scale Slumping in Moreux Crater: ESP_016642_2215 ESP_017710_2215 (Interval in Earth days: 83) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 41.13 | 44.1 | -7.3 | 6.121 | 42.8 | 41.2 |
| Aureum Chaos: ESP_016803_1770 ESP_088144_1770 (Interval in Earth days: 5559) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.11 | 334. | -3.6 | -16.2 | 51.1 | 57.8 |
| Pits along the Claritas Rupes: ESP_016450_1570 ESP_016516_1570 (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 | -22.5 | 252. | 7.58 | -14.9 | 58.8 | 60.8 |
| Gordii Dorsum: ESP_016847_1910 ESP_017559_1910 (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 | 10.61 | 211. | -2.9 | 6.107 | 44.9 | 47.3 |
| Candidate MSL Landing Site in Northeast Syrtis Major: ESP_016720_1980 ESP_016786_1980 (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 | 17.78 | 76.9 | 2.08 | -17.9 | 41.7 | 43.6 |
| Very Recent Small Impact Crater: ESP_016630_1720 ESP_030291_1720 (Interval in Earth days: 1064) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.08 | 17.6 | -3.5 | 8.058 | 52.4 | 48.4 |
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