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.
| Unusal Craters in Mud Flow from Galaxias Fossae: ESP_014344_2195 ESP_020436_2195 (Interval in Earth days: 474) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 39.00 | 139. | 1.68 | 16.67 | 61.3 | 64.9 |
| Western Edge of Layered Mound in Juventae Chasma: ESP_014378_1755 ESP_020470_1755 (Interval in Earth days: 475) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.47 | 297. | -4.8 | 16.67 | 35.3 | 53.4 |
| Gullies and Pasted on Material in Nereidum Montes: ESP_014391_1365 ESP_050192_1365 (Interval in Earth days: 2790) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -43.2 | 310. | -23. | 8.653 | 44.2 | 47.8 |
| Very Fresh 1-Kilometer Diameter Impact Crater: ESP_014405_1635 ESP_021776_1635 (Interval in Earth days: 575) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -16.2 | 281. | -5.4 | 26.42 | 33.9 | 41.2 |
| Exposures of Layered Rocks in Argyre Region: ESP_014167_1300 ESP_021947_1300 (Interval in Earth days: 606) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -49.7 | 302. | 8.10 | -18.2 | 43.7 | 44.1 |
| Ferric Oxide-Rich Deposit in East Candor Chasma: ESP_014154_1730 ESP_014431_1730 (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 | -6.75 | 292. | 5.69 | -21.1 | 35.2 | 35.9 |
| Hill and Adjacent Depression in Polar Layered Deposits: ESP_012815_1080 ESP_013013_1080 (Interval in Earth days: 15) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -71.7 | 141. | 1.59 | -20.3 | 57.3 | 57.1 |
| Fresh Central Pit Crater in Southern Highlands: ESP_012727_1540 ESP_013149_1540 (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 | -25.8 | 14.6 | -3.1 | -14.1 | 46.9 | 42.2 |
| Exposure of South Polar Layered Deposits with Minor Faulting: ESP_012855_1065 ESP_012723_1065 (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 | -73.2 | 132. | -7.1 | 7.21 | 58.4 | 58.8 |
| Gully and Fan in Southern Hemisphere Crater: ESP_013478_1300 ESP_021614_1300 (Interval in Earth days: 634) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -49.5 | 34.8 | -1.1 | -21.7 | 41.9 | 48.2 |
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