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.
| West Melas Chasma: ESP_041991_1715 ESP_042136_1715 (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 | -8.57 | 284. | -5.4 | 10.07 | 40.8 | 41.3 |
| Candidate ExoMars Landing Site in Hypanis Valles: ESP_041937_1920 ESP_042003_1920 (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 | 11.88 | 314. | 16.7 | -5.73 | 35.9 | 37.9 |
| Channel Containing Streamlined Forms Near Anseris Mons: ESP_041972_1490 ESP_042117_1490 (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 | -30.7 | 86.3 | -8.6 | 5.165 | 52.1 | 53.5 |
| Geologic Contact between Fluvial Deposits in Aeolis Dorsa: ESP_041943_1745 ESP_050303_1745 (Interval in Earth days: 652) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.30 | 154. | -6.0 | 6.611 | 39.3 | 31.5 |
| Banded Flow Terrain on Floor of Hellas Planitia: ESP_041960_1405 ESP_042039_1405 (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 | -39.1 | 54.6 | -1.8 | 27.31 | 57.1 | 56.6 |
| 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 |
| Possible Crater in South Polar Layered Deposits: ESP_041150_0920 ESP_041046_0920 (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 | -87.7 | 240. | 20.0 | 6.466 | 80.0 | 79.8 |
| 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 |
| 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 |
| Layered Crater Wall in Northwest Hellas Planitia: ESP_041116_1470 ESP_041393_1470 (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 | -32.6 | 56.9 | -0.3 | -23.1 | 40.2 | 45.4 |
Page 406 of 878 (8,777 images) | |||||