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.
| Eroded High-Latitude Mantle: PSP_007159_1405 PSP_007515_1405 (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 | -39.4 | 120. | 6.69 | -4.42 | 64.2 | 69.9 |
| Interior Channel in Durius Valles: PSP_007012_1630 PSP_007157_1630 (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 | -16.8 | 171. | -3.9 | 8.48 | 48.0 | 49.2 |
| Northwest Hellas Basin Landforms: PSP_007636_1400 ESP_016075_1400 (Interval in Earth days: 658) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.4 | 55.9 | 0.23 | -23.1 | 71.3 | 67.4 |
| Streamlined Form North of Mangala Valles: PSP_007683_1805 PSP_009542_1805 (Interval in Earth days: 145) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.500 | 207. | -3.0 | -16.3 | 47.1 | 56.6 |
| Naar Crater: PSP_007046_2030 ESP_025691_2030 (Interval in Earth days: 1453) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 22.90 | 317. | 3.89 | -21.5 | 39.0 | 42.0 |
| Possible Sulfates in Coprates Chasma: PSP_007205_1660 ESP_024505_1660 (Interval in Earth days: 1348) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.9 | 301. | 5.58 | -16.3 | 48.4 | 44.1 |
| Lobate Debris Aprons with Ridge-Like Structures: PSP_007693_2300 PSP_008550_2300 (Interval in Earth days: 67) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 49.57 | 286. | 6.42 | -7.47 | 45.2 | 44.0 |
| Fresh Rayed Crater: PSP_007707_1600 ESP_071927_1600 (Interval in Earth days: 5003) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -19.5 | 274. | -2.6 | 15.67 | 58.5 | 65.0 |
| Gullies: PSP_007031_2220 PSP_009826_2220 (Interval in Earth days: 218) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 41.43 | 4.84 | 2.91 | 18.33 | 45.6 | 45.0 |
| Gullies as Seen in MOC Image M02-02681: PSP_007213_1400 ESP_042618_1400 (Interval in Earth days: 2759) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.6 | 86.3 | 2.71 | 26.46 | 65.4 | 65.6 |
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