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.
| Excellent Exposure of Layered Mound in Terby Crater: ESP_013872_1520 ESP_014017_1520 (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 | -27.5 | 74.3 | 1.04 | 15.03 | 34.6 | 33.2 |
| Exposure of Layered Sequence in Terby Crater: ESP_013160_1530 ESP_074031_1530 (Interval in Earth days: 4743) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -26.9 | 74.0 | -8.4 | 2.702 | 41.5 | 52.0 |
| Light-Toned Outcrops along Ius Region Wallrock: ESP_012849_1705 ESP_013126_1705 (Interval in Earth days: 22) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.22 | 281. | -3.9 | -28.8 | 49.2 | 48.0 |
| Central Peak of Large Well-Preserved Crater: ESP_013198_1660 ESP_021545_1660 (Interval in Earth days: 651) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.7 | 113. | 8.48 | -27.9 | 42.6 | 48.8 |
| Gullies: ESP_014013_1265 ESP_014303_1265 (Interval in Earth days: 22) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -53.3 | 188. | 3.52 | 24.32 | 44.8 | 46.5 |
| Fresh Central Pit Crater in Southern Highlands: ESP_012727_1540 ESP_013149_1540 (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 | -25.8 | 14.6 | -3.1 | -14.1 | 46.9 | 42.2 |
| Gully and Fan in Southern Hemisphere Crater: ESP_013478_1300 ESP_021614_1300 (Interval in Earth days: 634) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -49.5 | 34.8 | -1.1 | -21.7 | 41.9 | 48.2 |
| Gullies: ESP_012722_1400 ESP_012867_1400 (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 | -39.6 | 153. | -6.2 | 7.111 | 47.5 | 44.4 |
| Light-Toned Fan-Like Features in Crater in Chryse Chaos: ESP_013256_1885 ESP_022104_1885 (Interval in Earth days: 689) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.534 | 327. | -1.4 | -13.8 | 53.6 | 52.2 |
| Terby Crater Surroundings: ESP_013885_1520 ESP_020465_1520 (Interval in Earth days: 513) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.9 | 79.1 | 4.84 | -7.13 | 34.3 | 58.0 |
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