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.
| Mesas with Circumferential Depressions Near Kasei Valles: ESP_011319_2100 ESP_011464_2100 (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 | 29.64 | 289. | -20. | -7.41 | 62.3 | 62.9 |
| Section of Wall Rock on the South Rim of Coprates Chasma: PSP_010501_1645 ESP_016026_1645 (Interval in Earth days: 431) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.4 | 305. | 5.32 | 23.12 | 62.0 | 48.0 |
| Ejecta and Interior of Gamboa Crater: PSP_010896_2210 ESP_028025_2210 (Interval in Earth days: 1335) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.80 | 315. | -8.5 | 7.506 | 58.9 | 49.2 |
| Possible MSL Landing Site in Holden Crater: ESP_011397_1535 ESP_011898_1535 (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 | -26.3 | 324. | 3.35 | 27.36 | 61.3 | 54.6 |
| Very Recent Small Crater: PSP_010772_2145 ESP_045136_2145 (Interval in Earth days: 2678) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 34.38 | 100. | 4.13 | -8.37 | 54.7 | 42.8 |
| Light-Toned Layering South of Ius Chasma with Unusual Morphology: PSP_010423_1720 ESP_016726_1720 (Interval in Earth days: 491) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.01 | 275. | -10. | 7.863 | 60.0 | 52.5 |
| Eastern Rim of Heimdal Crater: PSP_010648_2485 PSP_010846_2485 (Interval in Earth days: 15) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 68.34 | 235. | 11.9 | -10.7 | 63.8 | 68.8 |
| Phyllosilicate Ring in Terra Sirenum: PSP_010901_1510 ESP_055194_1510 (Interval in Earth days: 3452) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -28.9 | 187. | 0.35 | -23.2 | 66.4 | 62.6 |
| Very Fresh 1-Kilometer Impact Crater: ESP_011563_2200 ESP_011853_2200 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 39.70 | 104. | 4.18 | 26.78 | 66.9 | 68.9 |
| Outcrops of Light-Toned Materials Exposed in Highlands Crater Wall: PSP_010448_1530 ESP_016751_1530 (Interval in Earth days: 491) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -26.7 | 315. | -5.7 | 11.67 | 68.8 | 64.8 |
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