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.
| Well-Preserved Crater South of Hypanis Valles: ESP_039379_1890 ESP_056930_1890 (Interval in Earth days: 1368) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.936 | 313. | -2.4 | 22.35 | 56.9 | 52.3 |
| Candidate Landing Site for 2020 Mission in Firsoff Crater: ESP_039404_1820 ESP_047184_1820 (Interval in Earth days: 607) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.148 | 350. | 8.81 | -2.08 | 52.3 | 52.6 |
| Monitor Defrosting Patterns on Ridges in Region Dubbed Inca City: ESP_039473_0985 ESP_039776_0985 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -81.4 | 296. | -7.5 | 8.443 | 62.2 | 60.3 |
| Asimov Crater Gullies Present in MOC R1000011: ESP_039206_1320 ESP_039694_1320 (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 | -47.5 | 4.78 | -5.6 | -27.9 | 48.6 | 44.7 |
| Pits in Hale Crater Ejecta: ESP_039524_1445 ESP_039801_1445 (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 | -35.0 | 320. | -2.4 | -19.2 | 42.0 | 40.3 |
| A Triple-Crater in Elysium Planitia: ESP_039147_1940 ESP_039292_1940 (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 | 13.78 | 167. | -3.4 | 8.285 | 61.2 | 59.7 |
| Strange Flow: Landslide, Impact Melt or Lava?: ESP_039117_1745 ESP_039539_1745 (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 | -5.45 | 267. | 14.2 | -4.61 | 51.1 | 48.1 |
| Well-Preserved 30-Kilometer Impact Crater: ESP_039176_1615 ESP_039387_1615 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -18.5 | 98.5 | 6.16 | -4.52 | 47.3 | 45.5 |
| Osuga Valles Lowest Point: ESP_039181_1650 ESP_039326_1650 (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 | -14.7 | 322. | -5.4 | 7.662 | 49.0 | 46.3 |
| Well-Preserved Impact Crater on Floor of Coprates Chasma: ESP_039182_1675 ESP_048465_1675 (Interval in Earth days: 723) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.3 | 294. | -4.8 | 7.502 | 49.6 | 39.1 |
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