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.
| Outflow Channel Features in Arena Colles: ESP_035220_2085 ESP_036486_2085 (Interval in Earth days: 99) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 28.23 | 81.1 | 7.68 | -4.51 | 41.7 | 47.8 |
| Well Preserved Impact Crater: ESP_035166_1965 ESP_036089_1965 (Interval in Earth days: 72) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 16.19 | 117. | -0.1 | 20.79 | 45.6 | 46.4 |
| Light-Toned Deposits along Coprates Chasma Wallrock Slopes: ESP_035199_1655 ESP_035555_1655 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.1 | 300. | -5.2 | 4.733 | 62.5 | 62.8 |
| Meridiani Planum: ESP_034986_1785 ESP_042806_1785 (Interval in Earth days: 609) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.70 | 353. | 8.72 | -26.4 | 52.9 | 47.6 |
| Southern Capri Chasma: ESP_035225_1645 ESP_035858_1645 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.4 | 309. | 18.0 | 3.525 | 62.0 | 63.9 |
| Candidate Landing Site for 2020 Mission: ESP_035159_1945 ESP_036425_1945 (Interval in Earth days: 98) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 14.54 | 309. | -4.4 | -18.5 | 46.5 | 51.2 |
| Utopia Planitia Landform: ESP_035219_2025 ESP_069388_2025 (Interval in Earth days: 2663) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 22.40 | 110. | -4.8 | 5.209 | 44.1 | 47.6 |
| Impact Crater with Steep Slopes: ESP_035211_2105 ESP_035844_2105 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 30.39 | 324. | 23.3 | 12.21 | 39.9 | 42.9 |
| Possible Future Landing Site in McLaughlin Crater: ESP_035237_2020 ESP_036358_2020 (Interval in Earth days: 87) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.91 | 337. | 8.30 | -20.9 | 43.2 | 49.4 |
| Mesa-Plains Contact: ESP_035177_1835 ESP_035599_1835 (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 | 3.283 | 178. | 3.86 | -9.05 | 51.2 | 53.4 |
Page 468 of 878 (8,772 images) | |||||