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.
| Candidate Landing Site for 2020 Mission in Gusev Crater : ESP_055313_1655 ESP_055458_1655 (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 | -14.5 | 175. | -10. | 10.68 | 55.8 | 53.4 |
| Gully Comparison on Northern and Southern Rims of Asimov Crater : ESP_055570_1330 ESP_064247_1330 (Interval in Earth days: 676) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -46.6 | 4.45 | -8.2 | 25.99 | 65.1 | 67.5 |
| Landforms on the Floor of Barnard Crater: ESP_055502_1185 ESP_082036_1185 (Interval in Earth days: 2067) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -61.0 | 63.0 | 0 | 26.12 | 73.2 | 72.6 |
| Eastern Discontinuous Ejecta and Rays of Tomini Crater : ESP_055341_1965 ESP_064071_1965 (Interval in Earth days: 680) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 16.27 | 126. | 3.79 | -21.1 | 52.7 | 58.2 |
| Crater Breach and Associated Channels : ESP_055266_2210 ESP_055411_2210 (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 | 40.88 | 10.8 | -3.3 | 11.29 | 59.3 | 60.3 |
| Cones in Chryse Planitia : ESP_055413_1985 ESP_063299_1985 (Interval in Earth days: 614) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.53 | 321. | -7.2 | 3.32 | 54.6 | 50.0 |
| West of Erebus Montes : ESP_055220_2185 ESP_090048_2185 (Interval in Earth days: 2713) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 38.23 | 186. | 0 | -21.8 | 57.4 | 57.1 |
| Uplifted Blocks of Light-Toned Layered Deposits: ESP_054753_1825 ESP_055452_1825 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.261 | 340. | 0 | -23.2 | 51.3 | 54.5 |
| Ice Block Avalanche: ESP_054663_2650 ESP_063366_2650 (Interval in Earth days: 679) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 85.14 | 236. | 0 | 10.49 | 72.7 | 70.8 |
| Bang and Whoosh!: ESP_054066_1920 ESP_055200_1920 (Interval in Earth days: 88) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 11.79 | 14.7 | -2.8 | 15.56 | 47.4 | 50.4 |
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