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.
Central Uplift of an Impact Crater: ESP_017603_1550 ESP_026095_1550 (Interval in Earth days: 661) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -24.7 | 94.5 | 2.99 | -24.4 | 69.4 | 68.6 |
Well-Preserved 6-Kilometer Diameter Impact Crater: ESP_017334_2300 ESP_017413_2300 (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 | 49.67 | 230. | -12. | 9.171 | 44.2 | 42.2 |
Layered Deposits in Candor Chasma: ESP_017675_1760 ESP_017886_1760 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.13 | 285. | 5.36 | -4.03 | 55.6 | 56.7 |
Deflected Ejecta of Arabia Region Crater: ESP_017356_2175 ESP_024872_2175 (Interval in Earth days: 586) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 37.02 | 350. | 0 | 20.49 | 41.2 | 39.9 |
Terraced Pedestal Crater in CTX Image: ESP_017497_2325 ESP_017774_2325 (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 | 52.23 | 97.6 | 3.87 | -14.3 | 43.3 | 45.0 |
Lava Delta in Eastern Tharsis Region: ESP_017307_2050 ESP_017729_2050 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.97 | 249. | 4.76 | -11.9 | 41.7 | 44.1 |
Impact Crater Exposing Stratigraphy in Eos Chasma: ESP_017463_1630 ESP_018241_1630 (Interval in Earth days: 60) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -16.6 | 315. | 4.08 | -7.28 | 63.1 | 65.0 |
Hellas Planitia Terrain: ESP_017644_1420 ESP_025925_1420 (Interval in Earth days: 645) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.8 | 56.7 | 5.17 | -12.5 | 79.0 | 76.3 |
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 |
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 |
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