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.
Mounds in Oxia Colles: ESP_087801_2045 ESP_087735_2045 (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 | 24.18 | 335. | -9.3 | 8.282 | 44.6 | 42.9 |
Terrain Northeast of Airy Crater: ESP_087800_1780 ESP_088868_1780 (Interval in Earth days: 83) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.10 | 5.00 | 6.21 | -8.90 | 54.3 | 57.9 |
Crater in Arabia Terra: ESP_087747_2200 ESP_087681_2200 (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 | 39.57 | 7.75 | -7.8 | 6.691 | 43.3 | 42.0 |
Small Delta or Fan: ESP_087771_2065 ESP_087837_2065 (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 | 26.42 | 74.2 | -7.4 | -23.7 | 43.8 | 45.4 |
Crater with Evidence of Glacial Erosion: ESP_087913_2160 ESP_088124_2160 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.79 | 156. | -6.9 | -20.2 | 43.2 | 44.7 |
A Landslide by (Possible) Impact in Iani Chaos: ESP_087036_1790 ESP_086891_1790 (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 | -1.12 | 342. | -4.6 | -19.9 | 49.1 | 49.0 |
Margin of Lobate Deposit in Nereidum Montes: ESP_087406_1400 ESP_087116_1400 (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 | -39.7 | 323. | 21.8 | -7.50 | 75.8 | 74.4 |
Floor Unit in Coprates Chasma: ESP_087578_1655 ESP_087723_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 | -14.4 | 306. | 6.83 | 25.64 | 60.4 | 60.1 |
West Rim of Small Crater Within Stege Crater: ESP_087565_1840 ESP_088066_1840 (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 | 3.781 | 300. | -5.4 | 17.27 | 50.6 | 51.3 |
Hillslope Features: ESP_087431_2350 ESP_087919_2350 (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 | 54.77 | 349. | 3.83 | -10.2 | 46.5 | 46.4 |
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