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.
| Candidate Recent Impact Site : ESP_059279_1635 ESP_059635_1635 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -16.4 | 274. | -4.9 | 6.163 | 36.8 | 41.0 |
| Layer Orientations Within Nia Tholus : ESP_059384_1735 ESP_058883_1735 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.51 | 285. | 15.9 | -6.45 | 33.1 | 31.3 |
| Ancient Bedforms on Gordii Dorsum : ESP_059268_1895 ESP_059545_1895 (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 | 9.495 | 210. | 6.39 | -21.1 | 33.0 | 35.9 |
| Small Crater Northeast of Hellas Planitia : ESP_059352_1515 ESP_059286_1515 (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 | -28.3 | 83.6 | -7.9 | 13.60 | 44.4 | 42.0 |
| Gullies in Northwest Lowell Crater Wall Originating at Bouldery Deposit : ESP_059345_1285 ESP_058923_1285 (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 | -51.3 | 278. | -3.8 | 7.461 | 60.4 | 52.5 |
| Weathered Ejecta and Pitted Material Associated with Kontum Crater : ESP_059397_1480 ESP_051076_1480 (Interval in Earth days: 648) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -31.8 | 293. | 17.9 | 1.328 | 45.8 | 54.7 |
| Collapse Terrain South of Orson Welles Crater : ESP_059383_1780 ESP_060016_1780 (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 | -1.86 | 313. | -0.0 | -14.3 | 33.4 | 40.8 |
| Northern Argyre Planitia : ESP_059330_1385 ESP_059607_1385 (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 | -41.3 | 323. | 20.9 | -1.43 | 51.2 | 57.2 |
| Impact Crater with Central Pit : ESP_059263_1840 ESP_059408_1840 (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 | 4.060 | 349. | -8.6 | 7.628 | 33.4 | 32.6 |
| Large Channel East of Majuro Crater : ESP_059497_1465 ESP_059431_1465 (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 | -32.9 | 85.0 | -0.7 | 18.93 | 49.3 | 47.1 |
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