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.
| Newton Crater Valleys and Alluvial Fans: ESP_026012_1410 ESP_026078_1410 (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 | -38.7 | 199. | 4.09 | -15.0 | 76.7 | 78.1 |
| Well-Preserved Impact Crater on Floor of Coprates Chasma: ESP_025982_1675 ESP_025626_1675 (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 | -12.3 | 294. | 14.8 | 0 | 56.9 | 55.1 |
| Streamlined Forms in Elysium Planitia: ESP_025802_1960 ESP_026435_1960 (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 | 15.72 | 165. | 7.87 | -11.1 | 41.7 | 45.6 |
| Circular Depression and Mounds with Summit Depressions: ESP_025822_2165 ESP_027101_2165 (Interval in Earth days: 100) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.99 | 338. | -5.1 | 17.38 | 40.3 | 40.9 |
| Flows in Southern Elysium Planitia: ESP_025869_1855 ESP_034651_1855 (Interval in Earth days: 684) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 5.180 | 138. | 4.83 | 18.46 | 46.6 | 46.5 |
| Tharsis Region Lava Flow: ESP_026010_1940 ESP_025733_1940 (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 | 13.65 | 250. | -22. | 2.608 | 45.8 | 42.5 |
| Layered Flow Ejecta: ESP_026109_1575 ESP_026531_1575 (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 | -22.1 | 70.4 | -8.4 | -20.1 | 65.8 | 68.2 |
| Channel and Fan Near Equator: ESP_026199_1785 ESP_027676_1785 (Interval in Earth days: 116) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.50 | 130. | -6.3 | -21.0 | 52.7 | 55.8 |
| Light-Toned Hydrated Material along Melas Chasma Wallrock and Floor: ESP_026088_1710 ESP_026022_1710 (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 | -9.11 | 282. | -11. | 12.10 | 57.1 | 55.2 |
| Furthest Part of Young Channel in Lyot Crater: ESP_025899_2295 ESP_026031_2295 (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 | 49.20 | 30.5 | 20.2 | -6.05 | 40.6 | 42.7 |
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