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.
| Lobate Crater Ejecta: PSP_005867_1330 ESP_011431_1330 (Interval in Earth days: 434) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -46.4 | 118. | 0 | 14.15 | 48.3 | 67.4 |
| Bright Gully Deposits in A Fresh Impact Crater: PSP_006922_2120 PSP_007067_2120 (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 | 31.87 | 102. | 1.45 | 11.11 | 42.0 | 40.7 |
| Giza Region Unfrosted: PSP_004736_0950 PSP_005119_0950 (Interval in Earth days: 30) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -84.8 | 65.7 | 1.48 | -14.5 | 64.0 | 68.8 |
| Streamlined Hills in the Western Charitum Montes: PSP_006902_1275 ESP_011398_1275 (Interval in Earth days: 350) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -52.1 | 301. | -7.0 | 7.062 | 70.2 | 70.9 |
| Deeply-Incised Channels in Mantled Crater Walls: PSP_006544_1460 PSP_010750_1460 (Interval in Earth days: 328) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -33.6 | 351. | 0 | -16.0 | 50.6 | 71.0 |
| Lava Falls in Northern Kasei Valles: PSP_005610_2025 ESP_040659_2025 (Interval in Earth days: 2731) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 22.00 | 286. | -5.7 | 8.888 | 47.9 | 50.0 |
| Survey Layering and Faulting in Layered Deposits in Candor Chasma: PSP_006190_1725 ESP_049731_1725 (Interval in Earth days: 3393) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.54 | 293. | 0 | -22.8 | 34.9 | 32.5 |
| Hanging Valley in Minio Vallis: PSP_006470_1760 PSP_007762_1760 (Interval in Earth days: 101) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.14 | 208. | 0 | 23.15 | 36.5 | 48.2 |
| Dune Source in Newton Crater: PSP_006866_1375 ESP_015964_1375 (Interval in Earth days: 709) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -42.1 | 201. | -6.2 | 21.12 | 62.2 | 65.1 |
| Exposure of High-Latitude Polar Layered Deposits Not Well Observed: PSP_005157_0875 PSP_005577_0925 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.2 | 152. | 0 | 14.21 | 71.5 | 75.0 |
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