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.
Lineated Valley Fill in Nilosyrtis Region: ESP_014307_2130 ESP_020188_2130 (Interval in Earth days: 458) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 32.47 | 70.8 | -0.7 | 24.40 | 56.9 | 58.3 |
Possible Region of Past Ponded Water: ESP_014407_2045 ESP_020288_2045 (Interval in Earth days: 458) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.15 | 221. | 5.35 | 29.18 | 49.2 | 56.3 |
Central Uplift of a Large Crater North of Hellas Planitia: ESP_014439_1505 ESP_020742_1505 (Interval in Earth days: 491) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -29.2 | 74.5 | 5.54 | 18.53 | 36.0 | 53.2 |
Small Crater on Lobate Apron: ESP_014398_1305 ESP_020490_1305 (Interval in Earth days: 475) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -49.4 | 118. | -7.6 | 7.572 | 47.0 | 64.0 |
Multiple Branches of the Cerberus Fossae: ESP_014383_1910 ESP_022097_1910 (Interval in Earth days: 601) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 10.66 | 158. | 0.24 | -14.4 | 41.3 | 53.7 |
Exposures of Layered Rocks in Argyre Region: ESP_014167_1300 ESP_021947_1300 (Interval in Earth days: 606) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -49.7 | 302. | 8.10 | -18.2 | 43.7 | 44.1 |
Ferric Oxide-Rich Deposit in East Candor Chasma: ESP_014154_1730 ESP_014431_1730 (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 | -6.75 | 292. | 5.69 | -21.1 | 35.2 | 35.9 |
Exposure of Thick Layered Deposits in Hebes Chasma: ESP_013205_1790 ESP_021565_1790 (Interval in Earth days: 651) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.82 | 283. | -25. | -3.43 | 50.5 | 51.4 |
Eastern Tooting Crater Impact Processes: ESP_013735_2035 ESP_014157_2035 (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 | 23.18 | 207. | 6.42 | -8.32 | 57.4 | 52.6 |
Crater in the Sirenum Fossae Region: ESP_012918_1450 ESP_013340_1450 (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 | -34.4 | 201. | -7.6 | -20.0 | 44.4 | 40.3 |
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