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.
| Equatorial-Facing Trough Slope Exposure of North Polar Layered Deposits: ESP_079448_2670 ESP_079515_2670 (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 | 86.93 | 101. | -6.8 | -20.7 | 61.8 | 62.5 |
| Small Impact into Debris Covered Glacier: ESP_079641_2215 ESP_079918_2215 (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 | 41.27 | 273. | 8.68 | -5.04 | 43.6 | 45.8 |
| Possible Abalos Mensae Dune Source: ESP_079495_2625 ESP_079455_2625 (Interval in Earth days: 3) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 82.34 | 284. | -6.8 | 8.806 | 58.8 | 58.0 |
| Fresh Crater Surrounded by Amazonis Planitia Lava Plains with Asymmetry: ESP_079697_2115 ESP_079763_2115 (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 | 31.09 | 186. | 9.02 | -7.51 | 44.3 | 46.0 |
| Scalloped Cliff Formations : ESP_079343_2640 ESP_079237_2640 (Interval in Earth days: 8) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 83.86 | 111. | -8.8 | 5.451 | 59.9 | 59.4 |
| Erosional Features in Crater in Medusae Fossae Formation: ESP_079222_1720 ESP_079367_1720 (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 | -7.83 | 199. | -7.0 | 11.39 | 60.4 | 59.8 |
| Fissure and Channel Source Region: ESP_079168_1955 ESP_079313_1955 (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 | 15.52 | 231. | -12. | 4.368 | 48.8 | 47.9 |
| Pit in Hephaestus Fossae: ESP_079251_1985 ESP_079396_1985 (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 | 18.40 | 124. | -5.0 | 11.77 | 47.4 | 46.5 |
| Layered Deposits: ESP_079096_2225 ESP_079241_2225 (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 | 42.08 | 32.5 | 0.36 | 11.98 | 43.4 | 42.5 |
| Maja Valles: ESP_079363_1980 ESP_079640_1980 (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 | 17.80 | 306. | 5.62 | -15.7 | 47.1 | 49.6 |
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