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.
| 25-Kilometer Diameter Gullied Impact Crater in Acidalia Planitia: ESP_016592_2170 ESP_016737_2170 (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 | 36.54 | 329. | -3.7 | 9.38 | 41.6 | 40.3 |
| Possible Phyllosilicate-Rich Area in Syrtis Major: ESP_016628_2040 ESP_017340_2040 (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 | 23.69 | 68.6 | -7.2 | 6.233 | 41.2 | 42.0 |
| Fretted Valley Outlet: ESP_016391_2195 ESP_016668_2195 (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 | 38.96 | 56.1 | -0.8 | -19.4 | 42.2 | 43.3 |
| Well-Preserved Crater in Margaritifer Terra: ESP_016407_1675 ESP_016763_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 | -12.5 | 345. | -0.5 | 12.61 | 52.5 | 55.3 |
| Southern Margin of Mantle Material within Crater: ESP_016542_1435 ESP_025403_1435 (Interval in Earth days: 690) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -36.1 | 262. | 6.93 | 27.81 | 69.4 | 67.9 |
| Crater with Sharp Rim and Elongated Secondaries: ESP_016810_2260 ESP_017232_2260 (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 | 45.63 | 135. | 1.70 | -9.75 | 42.9 | 43.1 |
| Unnamed Crater in Polygonal Terrain in Western Utopia Planitia: ESP_016469_2260 ESP_016535_2260 (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 | 45.59 | 84.3 | 8.50 | -5.58 | 43.4 | 44.2 |
| Crossing Wrinkle Ridges and Secondaries in Hesperia Planum: ESP_016310_1545 ESP_016666_1545 (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 | -25.2 | 115. | 3.44 | 15.21 | 59.1 | 62.7 |
| Chlorides in Dune Materials in Noachis Terra: ESP_016380_1520 ESP_019716_1520 (Interval in Earth days: 260) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.6 | 5.67 | -8.5 | 15.10 | 62.3 | 63.2 |
| Well-Preserved Impact Crater on Somewhat Older Crater: ESP_016345_2210 ESP_017624_2210 (Interval in Earth days: 99) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.46 | 231. | -0.3 | 11.17 | 42.8 | 40.6 |
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