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.
| Hydaspis Chaos: ESP_067374_1825 ESP_074852_1825 (Interval in Earth days: 582) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.223 | 335. | -5.0 | -17.0 | 41.3 | 52.8 |
| Terrain Sample Northwest of Sytinskaya Crater: ESP_067520_2235 ESP_068061_2235 (Interval in Earth days: 42) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 43.15 | 305. | 4.04 | 14.32 | 62.6 | 55.5 |
| Feature near South Polar Residual Cap: ESP_067540_0920 ESP_067565_0920 (Interval in Earth days: 2) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.7 | 182. | 13.4 | 27.64 | 79.9 | 79.0 |
| Edge of South Polar Residual Cap: ESP_067636_0920 ESP_058933_0920 (Interval in Earth days: 678) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -88.1 | 45.8 | 29.4 | 19.28 | 80.4 | 82.9 |
| Gullied Slope: ESP_067497_1470 ESP_073920_1470 (Interval in Earth days: 501) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -32.8 | 223. | 6.55 | 21.01 | 42.8 | 52.4 |
| Candidate ExoMars Landing Site in Oxia Planum: ESP_067519_1980 ESP_076830_1980 (Interval in Earth days: 725) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.84 | 336. | 8.05 | -2.37 | 46.3 | 40.9 |
| Crater near Uranius Mons: ESP_067495_2080 ESP_067363_2080 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 27.80 | 271. | -7.2 | 8.657 | 53.2 | 53.7 |
| Stratified Mound near Oxia Planum: ESP_067440_2000 ESP_067572_2000 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 19.83 | 332. | -4.1 | -19.5 | 48.9 | 48.9 |
| Oyama Crater Rim: ESP_067664_2045 ESP_067796_2045 (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 | 24.09 | 339. | 7.76 | -5.86 | 48.5 | 48.5 |
| Utopia Planitia: ESP_067580_2050 ESP_067844_2050 (Interval in Earth days: 20) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.87 | 110. | 15.7 | -11.2 | 49.1 | 48.9 |
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