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.
| Pit in Eastern Noctis Labyrinthus with Jarosite : ESP_043363_1725 ESP_043719_1725 (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 | -7.65 | 267. | -24. | -11.6 | 54.6 | 55.6 |
| Dark Dunes Superimposed on Light Bedforms in MOC E01-01076 : ESP_043442_1730 ESP_044009_1730 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.73 | 267. | 5.82 | 18.1 | 52.5 | 54.1 |
| Layered Bedrock in Terby Crater : ESP_043225_1525 ESP_043937_1525 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.3 | 75.1 | -0.4 | 23.99 | 65.1 | 68.0 |
| Braided Channel in the Southern Highlands : ESP_043261_1440 ESP_045226_1440 (Interval in Earth days: 153) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -35.7 | 174. | -6.7 | -21.5 | 71.8 | 74.2 |
| Possible Crustal Carbonate Remnant Butte : ESP_043322_2295 ESP_043599_2295 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 49.16 | 296. | 0.31 | -15.7 | 42.9 | 43.3 |
| Landslides in Trough South of Ius Chasma : ESP_043376_1710 ESP_043943_1710 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.90 | 270. | -2.0 | 9.783 | 53.9 | 55.9 |
| Holden Crater Dune Topography : ESP_043229_1540 ESP_043374_1540 (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 | -25.7 | 326. | -7.9 | 7.843 | 64.3 | 64.6 |
| Infilled Crater with Overlying Secondary Craters in Arcadia Planitia : ESP_043260_2265 ESP_043972_2265 (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 | 46.21 | 189. | 0.67 | 17.69 | 42.2 | 39.1 |
| Intercrater Terrain in Terra Sabaea : ESP_043292_1550 ESP_044413_1550 (Interval in Earth days: 88) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -24.6 | 44.9 | 7.30 | -23.9 | 63.3 | 69.4 |
| InSight Mission Candidate Landing Site : ESP_043183_1845 ESP_043671_1845 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.459 | 135. | 21.3 | -10.5 | 43.7 | 48.4 |
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