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.
| Pedestal Crater: ESP_041888_2270 ESP_041954_2270 (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 | 46.82 | 208. | 1.80 | -12.8 | 52.5 | 52.8 |
| Clay-Rich Terrain in Oxia Planum: A Proposed ExoMars Landing Site: ESP_039154_1985 ESP_065448_1985 (Interval in Earth days: 2049) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.27 | 335. | -1.2 | -20.7 | 63.6 | 66.4 |
| Candidate Landing Site for 2020 Mission in Oxia Palus Region: ESP_041211_1980 ESP_049927_1980 (Interval in Earth days: 679) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.65 | 336. | 10 | 27.09 | 41.0 | 38.3 |
| Light-Toned Hydrated Materials along Northern Melas Chasma Wallrock: ESP_041279_1720 ESP_042057_1720 (Interval in Earth days: 61) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.90 | 284. | -4.4 | -27.6 | 34.7 | 43.1 |
| Triple Crater: ESP_041350_1455 ESP_049987_1450 (Interval in Earth days: 673) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -34.4 | 148. | 6.43 | -12.8 | 43.7 | 40.2 |
| Light-Toned Layered Deposits Exposed along the Floor of Coprates Chasma: ESP_041186_1660 ESP_041964_1660 (Interval in Earth days: 61) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.0 | 304. | -7.9 | -26.5 | 35.1 | 44.3 |
| Light-Toned Hydrated Materials Inside Ius Chasma: ESP_041121_1725 ESP_048136_1725 (Interval in Earth days: 547) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.24 | 276. | 1.18 | 20.39 | 33.8 | 43.6 |
| Wrinkle Ridge Near Ganges Catena: ESP_041226_1770 ESP_041160_1770 (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 | -2.83 | 290. | -2.8 | 18.39 | 34.6 | 33.0 |
| Small Feature on South Polar Layered Deposits: ESP_041111_0925 ESP_041004_0925 (Interval in Earth days: 8) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.2 | 244. | 7.47 | 28.48 | 80.0 | 76.6 |
| Ridges and Light-Toned Outcrops North of Atlantis Chaos: ESP_041151_1500 ESP_047309_1500 (Interval in Earth days: 480) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -29.7 | 181. | -8.0 | 2.323 | 39.6 | 50.5 |
Page 424 of 896 (8,955 images) | |||||