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.
| Channels on Alba Mons : ESP_044814_2270 ESP_045157_2270 (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 | 46.47 | 246. | 6.41 | -14.1 | 41.6 | 45.4 |
| Rim and Ejecta of Well-Preserved Impact Crater : ESP_044978_1610 ESP_045255_1610 (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 | -18.7 | 98.7 | 4.23 | -8.51 | 62.3 | 61.9 |
| Climbing Dunes on Crater Wall : ESP_044765_1895 ESP_045187_1895 (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 | 9.263 | 150. | -1.9 | 8.506 | 46.9 | 46.0 |
| Fractures and Exposed Bedrock in Lyot Crater : ESP_044756_2300 ESP_045099_2300 (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 | 49.56 | 28.7 | 8.24 | -10.8 | 42.1 | 45.7 |
| Crater Adjacent to Scarp in North Tempe Terra : ESP_044681_2290 ESP_044826_2290 (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 | 48.77 | 278. | -8.4 | 5.512 | 42.9 | 42.4 |
| Transverse Aeolian Ridges in Scandia Cavi : ESP_044722_2570 ESP_044405_2570 (Interval in Earth days: 25) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 76.93 | 226. | 2.31 | 28.96 | 55.5 | 52.8 |
| North Polar Dune Changes : ESP_044911_2590 ESP_045003_2590 (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 | 78.61 | 105. | 3.33 | 19.78 | 57.6 | 57.4 |
| Inflated Lava Flows in Eastern Tharsis Region : ESP_044933_1740 ESP_045078_1740 (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 | -6.13 | 246. | -7.9 | 18.07 | 55.2 | 53.2 |
| Troughs within East Candor Chasma : ESP_044773_1735 ESP_045406_1735 (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 | -6.63 | 292. | 13.5 | 29.45 | 54.4 | 51.4 |
| 30-Meter Diameter Pit Near Kasei Valles : ESP_044879_1955 ESP_051327_1955 (Interval in Earth days: 502) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 15.46 | 277. | 3.25 | -25.6 | 44.1 | 38.6 |
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