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 in Northern Meridiani Planum : ESP_028340_1865 ESP_060001_1865 (Interval in Earth days: 2467) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 6.308 | 1.62 | 5.28 | -12.5 | 51.8 | 38.1 |
| Faulted Plains in Tempe Terra : ESP_028277_2260 ESP_028409_2260 (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 | 45.63 | 275. | 8.54 | -16.9 | 53.5 | 57.4 |
| Deep Bedrock in Juventae Chasma : ESP_028527_1750 ESP_034632_1750 (Interval in Earth days: 476) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.70 | 298. | 3.46 | 18.38 | 54.7 | 51.8 |
| West Candor Chasma Layering : ESP_028422_1730 ESP_026378_1730 (Interval in Earth days: 160) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.73 | 284. | 8.76 | -8.93 | 55.0 | 56.8 |
| Possible Repetitive Bedding in Terra Sirenum Hills : ESP_028319_1445 ESP_028174_1445 (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 | -35.3 | 220. | 5.27 | -13.6 | 69.1 | 71.5 |
| Layered Bedrock in Gusev Crater : ESP_028492_1645 ESP_033819_1645 (Interval in Earth days: 415) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.1 | 175. | -6.9 | 16.51 | 59.0 | 49.8 |
| Gamboa Crater : ESP_028447_2210 ESP_033339_2210 (Interval in Earth days: 381) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.75 | 315. | 6.03 | -8.84 | 54.5 | 46.6 |
| Candidate Future Landing Site in Trouvelot Crater : ESP_028512_1960 ESP_027114_1960 (Interval in Earth days: 109) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 15.85 | 346. | -13. | 15.53 | 53.2 | 45.0 |
| Crater Near Athabasca Valles Source : ESP_028453_1900 ESP_028809_1900 (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 | 9.914 | 157. | -6.5 | 3.145 | 52.6 | 53.5 |
| Potential Future Landing Site in Eastern Terby Crater : ESP_028377_1520 ESP_028654_1520 (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 | -27.5 | 75.0 | 13.9 | -7.90 | 63.9 | 63.2 |
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