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.
| Light-Toned Deposits North of Eberswalde Crater: ESP_033418_1565 ESP_033563_1565 (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 | -23.3 | 326. | -6.7 | 8.036 | 50.7 | 51.9 |
| Floor of Mclaughlin Crater: ESP_033391_2020 ESP_037149_2020 (Interval in Earth days: 293) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.90 | 337. | 1.00 | 18.02 | 38.3 | 51.1 |
| Lava-Embayed Crater in Kasei Valles: ESP_033590_2055 ESP_034078_2055 (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 | 25.39 | 301. | 26.4 | 0.83 | 36.7 | 39.6 |
| Candidate New Impact Site: ESP_033494_1900 ESP_089763_1900 (Interval in Earth days: 4384) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.663 | 47.0 | 1.35 | 10.81 | 37.9 | 52.5 |
| Dunes in Crater North of Antoniadi Crater: ESP_033454_2065 ESP_033955_2065 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 26.14 | 57.0 | 1.01 | 22.61 | 39.2 | 37.5 |
| Channels and Central Pit of Terra Cimmeria Crater: ESP_033556_1435 ESP_042299_1435 (Interval in Earth days: 681) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -36.3 | 158. | 21.1 | 1.451 | 59.8 | 60.1 |
| Pit or Crater near Galaxias Chaos: ESP_033332_2155 ESP_042088_2155 (Interval in Earth days: 683) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.10 | 146. | 0.31 | 28.38 | 43.1 | 41.8 |
| Southern Uzboi Vallis Region: ESP_033484_1480 ESP_033629_1480 (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 | -31.7 | 324. | 10.4 | 23.41 | 56.2 | 57.6 |
| Gullies in Central Peak of Hale Crater: ESP_033695_1445 ESP_024346_1445 (Interval in Earth days: 729) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -35.3 | 323. | 18.6 | -1.51 | 61.4 | 53.6 |
| Layered Light-Toned Crater-Filling Material in Northwest Hellas Region: ESP_033520_1545 ESP_033454_1545 (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 | -25.2 | 62.0 | -3.2 | 18.61 | 53.2 | 50.8 |
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