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.
Mesa Armored by Impact Ejecta in Ganges Chasma: ESP_011371_1730 ESP_011516_1730 (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 | -7.13 | 312. | 0.00 | 16.31 | 57.8 | 56.3 |
Gullies on Pole-Facing Slope and Arcuate Ridges on Crater Floor: ESP_011995_1410 ESP_012496_1410 (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 | -38.8 | 201. | -5.2 | 16.43 | 58.2 | 49.0 |
Layers with Iron Magnesium Phyllosilicate on Crater Floor: PSP_010419_2140 PSP_010841_2140 (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 | 33.71 | 17.1 | 16.6 | 1.275 | 49.7 | 55.7 |
Depression in Avernus Cavi Region: PSP_010875_1785 ESP_045529_1785 (Interval in Earth days: 2701) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.65 | 173. | -1.3 | 29.84 | 57.1 | 48.6 |
Collapse Pit in Tractus Fossae: ESP_011386_2065 ESP_011531_2065 (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 | 26.14 | 259. | -6.1 | 8.253 | 61.0 | 61.3 |
Uplift in Oudemans Crater: ESP_011966_1700 ESP_012467_1700 (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 | -9.73 | 268. | 2.38 | 27.90 | 55.8 | 50.3 |
Western Half of Very Fresh Crater in Utopia Region: PSP_010402_2050 ESP_053495_2050 (Interval in Earth days: 3357) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.57 | 124. | -2.7 | -23.1 | 51.1 | 44.1 |
Stratigraphy of Primary Mesa in Terby Crater: PSP_010826_1525 ESP_016272_1525 (Interval in Earth days: 424) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.1 | 74.2 | 4.13 | -10.0 | 65.9 | 60.7 |
Knobs and Thermokarst: ESP_011365_1365 ESP_011642_1365 (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 | -43.3 | 120. | 5.79 | -16.4 | 67.6 | 65.5 |
Erosional Remnants on Ganges Mensa: ESP_011582_1730 ESP_011648_1730 (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 | -7.16 | 311. | 6.37 | -16.2 | 57.0 | 58.6 |
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