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.
| Lyot Crater Rim : ESP_051072_2315 ESP_051006_2315 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 51.30 | 32.4 | -8.2 | 4.828 | 50.8 | 50.6 |
| Degraded Crater Rim Morphology : ESP_050902_1785 ESP_050968_1785 (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 | -1.24 | 0.00 | 0.19 | -22.7 | 36.1 | 38.6 |
| Floor of Ius Chasma : ESP_051050_1725 ESP_051195_1725 (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 | -7.56 | 279. | 7.85 | 22.39 | 39.4 | 40.0 |
| Lyot Crater Rim with Phyllosilicate Detection : ESP_050927_2295 ESP_050861_2295 (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 | 49.37 | 31.6 | -8.4 | 5.371 | 51.0 | 50.8 |
| Knobs in Adamas Labyrinthus : ESP_051109_2170 ESP_051188_2170 (Interval in Earth days: 7) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.72 | 103. | 3.35 | 29.07 | 41.2 | 38.6 |
| Gully Monitoring : ESP_050991_2350 ESP_051281_2350 (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 | 54.56 | 83.3 | -8.7 | 7.025 | 53.8 | 49.8 |
| Central Nirgal Vallis : ESP_050930_1515 ESP_033603_1515 (Interval in Earth days: 1350) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -28.1 | 318. | 5.52 | -25.6 | 49.5 | 57.7 |
| Hale Crater Ejecta with Pits and Rocky Outcrops : ESP_051154_1455 ESP_050521_1455 (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 | -34.1 | 324. | -8.4 | 17.88 | 58.0 | 46.3 |
| Mesa in Utopia Planitia : ESP_050951_2110 ESP_060393_2110 (Interval in Earth days: 736) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 30.54 | 98.0 | -0.1 | -20.0 | 39.5 | 40.2 |
| Athabasca Valles Lava Contact Relation: ESP_051002_1840 ESP_053204_1840 (Interval in Earth days: 172) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.995 | 149. | -1.3 | 7.887 | 35.9 | 49.0 |
Page 329 of 891 (8,901 images) | |||||