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.
| Layers on Hellas Planitia Rim and Proposed Site for Future Exploration: ESP_023195_1505 ESP_023340_1505 (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 | -29.1 | 66.7 | -12. | 6.662 | 35.1 | 34.9 |
| The 2-Kilometer Diameter Well-Preserved Vaduz Crater: ESP_023302_2185 ESP_023579_2185 (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 | 38.23 | 15.8 | 1.32 | -22.4 | 57.8 | 55.3 |
| Crater with Rugged Floor in THEMIS V26860010: ESP_023396_1490 ESP_024319_1490 (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 | -30.8 | 338. | 2.17 | 16.49 | 36.5 | 49.0 |
| Small Mounds in Chryse Planitia: ESP_023159_1995 ESP_023225_1995 (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 | 19.36 | 322. | -2.4 | -20.9 | 45.9 | 46.3 |
| Polar Layers Exposed on Promethei Lingula Surface: ESP_023102_0980 ESP_022983_0980 (Interval in Earth days: 9) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -82.0 | 111. | -8.0 | 6.991 | 70.0 | 67.3 |
| Bedrock Exposed in Rim and Terraces of Crater in Molesworth Crater: ESP_023126_1520 ESP_023627_1520 (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 | -27.4 | 149. | -7.8 | 15.53 | 33.7 | 36.6 |
| Boundary between Ophir and Candor Chasmata: ESP_023134_1755 ESP_023635_1755 (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 | -4.67 | 287. | 4.94 | 27.71 | 32.9 | 30.0 |
| Pitted Materials in Bakhuysen Crater: ESP_020309_1570 ESP_020731_1570 (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 | -22.8 | 16.2 | 8.95 | -6.93 | 57.0 | 54.4 |
| A Pedestal Crater in Malea Planum: ESP_022787_1085 ESP_030580_1085 (Interval in Earth days: 607) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -71.3 | 55.1 | -4.6 | 21.88 | 56.9 | 53.9 |
| Wrinkle Ridges in West Meridiani Planum: ESP_022749_1855 ESP_022960_1855 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 5.439 | 357. | 5.12 | -4.25 | 41.4 | 39.6 |
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