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.
Layering in Southern Lucus Planum: ESP_089336_1720 ESP_089481_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 | -7.84 | 187. | 4.06 | 19.82 | 59.8 | 58.4 |
Characterize Possilbe Rotorcraft Landing Site: ESP_089283_2205 ESP_089362_2205 (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 | 39.97 | 189. | -7.1 | 19.14 | 48.3 | 46.5 |
Features around Crater in Arabia Terra: ESP_089592_2190 ESP_089104_2190 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 38.44 | 34.3 | -16. | 10.19 | 51.6 | 45.4 |
Channelized Flow in Arcadia Planitia: ESP_089587_2285 ESP_089455_2285 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 48.17 | 169. | -17. | 9.076 | 53.4 | 49.7 |
Possible Vent in Young Lava Flows in Elysium Region: ESP_089244_2090 ESP_089534_2090 (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 | 28.68 | 174. | 4.31 | 28.13 | 47.1 | 46.6 |
Planned ExoMars Landing Ellipse Imaging in Oxia Planum: ESP_089581_1995 ESP_089291_1995 (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 | 19.24 | 335. | 3.28 | -24.9 | 50.3 | 51.5 |
Potential Compound Dune: ESP_089573_2610 ESP_089389_2610 (Interval in Earth days: 14) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 80.87 | 160. | 19.2 | -5.86 | 64.3 | 63.7 |
Positive Relief Material in Association with Osuga Valles Depression: ESP_089397_1655 ESP_089542_1655 (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 | -14.5 | 323. | -1.7 | 14.98 | 63.7 | 62.2 |
Potential Compound Dune: ESP_089362_2590 ESP_089415_2590 (Interval in Earth days: 4) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 78.72 | 174. | 6.27 | -7.76 | 61.5 | 63.0 |
Features around Crater in Terra Sabaea: ESP_089319_2205 ESP_089385_2205 (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 | 39.93 | 284. | 8.56 | -7.88 | 47.1 | 49.1 |
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