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.
| Exposure of North Polar Layered Deposits : ESP_045625_2615 ESP_045599_2615 (Interval in Earth days: 2) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 81.24 | 44.7 | 8.37 | -6.57 | 66.3 | 66.7 |
| Fractured Crater Fill : ESP_045522_2175 ESP_045588_2175 (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 | 36.97 | 1.48 | 8.69 | -9.68 | 44.3 | 46.6 |
| Breached Crater Near Marte Vallis : ESP_045634_2035 ESP_045924_2035 (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 | 23.36 | 185. | 6.26 | 26.04 | 44.5 | 45.0 |
| Buried Crater in Athabasca Valles Lava : ESP_045530_1855 ESP_046598_1855 (Interval in Earth days: 83) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 5.431 | 148. | -1.4 | 11.56 | 48.3 | 50.4 |
| On the Shape of Impact Craters: ESP_044998_1745 ESP_046409_1745 (Interval in Earth days: 110) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.41 | 271. | 0 | -14.4 | 54.1 | 53.0 |
| Bedrock Exposures on the Floor of Bakhuysen Crater: ESP_044981_1560 ESP_051785_1560 (Interval in Earth days: 530) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -23.6 | 16.0 | 20.2 | -3.50 | 64.6 | 58.9 |
| Candidate Landing Site for 2020 Mission in Eberswalde Crater : ESP_045062_1555 ESP_045128_1555 (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 | -24.0 | 327. | -2.3 | -19.9 | 65.9 | 66.7 |
| Ice-Dune Interactions in Olympia Undae : ESP_045170_2620 ESP_045144_2620 (Interval in Earth days: 2) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 81.93 | 225. | 7.58 | -6.71 | 61.7 | 62.2 |
| Candidate Human Exploration Zone Near Gusev Crater : ESP_045239_1650 ESP_053045_1650 (Interval in Earth days: 608) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.8 | 173. | 5.61 | -6.50 | 58.6 | 61.3 |
| Candidate Landing Site for 2020 Mission : ESP_045318_1655 ESP_044962_1655 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.5 | 175. | 26.7 | -3.09 | 56.6 | 60.0 |
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