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.
Possible Clay Beds in West Ladon Valles Channels: ESP_017489_1610 ESP_035119_1610 (Interval in Earth days: 1374) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -18.9 | 326. | -5.8 | -19.4 | 65.4 | 66.3 |
Streamlined Landform with Benches in Kasei Valles System: ESP_017398_1970 ESP_017820_1970 (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 | 16.92 | 285. | 9.39 | -8.3 | 43.9 | 46.4 |
Light-Toned Layering in Noctis Region Pit: ESP_017399_1680 ESP_027236_1680 (Interval in Earth days: 766) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.8 | 263. | -4.9 | -24.5 | 60.2 | 62.0 |
Light-Toned Layered Deposits on Northern Edge of Hellas Planitia: ESP_017459_1500 ESP_018870_1500 (Interval in Earth days: 110) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -29.5 | 66.7 | 3.18 | -25.8 | 72.3 | 72.8 |
Sinuous Ridge Witin the Upper Reach of Maadim Vallis: ESP_017600_1540 ESP_017745_1540 (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 | -25.9 | 176. | 0 | 13.55 | 70.4 | 70.0 |
Bacolor Crater Gullies: ESP_017681_2135 ESP_017971_2135 (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 | 32.97 | 118. | -8.0 | 14.61 | 42.4 | 41.1 |
Spillway in Central Valles Marineris: ESP_017609_1750 ESP_018031_1750 (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 | -5.05 | 287. | 6.19 | -11.7 | 56.0 | 58.0 |
Laminar Flow in Ejecta Layer North of Tooting Crater: ESP_017625_2040 ESP_018258_2040 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.80 | 207. | 2.38 | -18.9 | 42.9 | 46.3 |
Alba Region Valleys: ESP_017676_2260 ESP_017742_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 | 45.51 | 251. | 7.35 | -8.07 | 41.6 | 42.9 |
Olympica Fossae: ESP_017439_2050 ESP_018639_2050 (Interval in Earth days: 93) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.61 | 245. | 8.39 | -13.2 | 41.8 | 46.9 |
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