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 Chryse Planitia : ESP_058974_2245 ESP_059475_2245 (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 | 44.03 | 313. | -3.7 | 11.54 | 56.2 | 49.1 |
| Landslide in Hydraotes Chaos : ESP_058776_1815 ESP_058842_1815 (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 | 1.538 | 324. | 11.2 | -12.9 | 31.2 | 32.9 |
| Candidate Mars 2020 Landing Site in Gusev Crater : ESP_058742_1645 ESP_066562_1645 (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 | -15.2 | 175. | 0.28 | -10.4 | 30.7 | 41.2 |
| Valley-Channel Transitions in Crater in Arabia Terra : ESP_058721_1875 ESP_067372_1875 (Interval in Earth days: 674) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.534 | 26.2 | -2.4 | 29.70 | 34.8 | 40.7 |
| Scalloped Depressions in Amphitrites Patera : ESP_058997_1220 ESP_058931_1220 (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 | -57.6 | 61.2 | -8.2 | 5.8 | 59.5 | 57.7 |
| Pitted Cones in Chryse Planitia : ESP_058723_2160 ESP_059000_2160 (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 | 35.84 | 327. | 4.89 | -20.5 | 52.8 | 50.7 |
| Hunt for Ancient Impact Craters Near Nili Fossae : ESP_058772_2025 ESP_058706_2025 (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 | 22.32 | 72.3 | -7.1 | 14.88 | 43.0 | 42.4 |
| Glacier Moving Upslope Near Reull Vallis : ESP_058916_1370 ESP_059338_1370 (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 | -42.7 | 108. | 4.53 | -8.97 | 46.2 | 54.0 |
| Troughs in Acidalia Planitia : ESP_058987_2245 ESP_058565_2245 (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 | 43.98 | 319. | -7.2 | 8.327 | 56.1 | 61.5 |
| Crater Breach and Kasei Valles Lava Flow : ESP_058830_2040 ESP_058540_2040 (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 | 23.79 | 287. | 7.29 | -13.5 | 42.5 | 47.1 |
Page 260 of 878 (8,771 images) | |||||