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 Debris Apron with Ridge-Like Structures in Tempe Terra: PSP_008563_2320 PSP_008774_2320 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 51.77 | 288. | 6.33 | -7.60 | 43.4 | 44.6 |
| Curving Channel Near Rahway Valles: PSP_008607_1900 PSP_009042_1900 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 10.11 | 175. | -8.0 | 8.124 | 48.9 | 49.1 |
| Northern Hemisphere Polygons and Seasonal Spots: PSP_009159_2650 PSP_009753_2650 (Interval in Earth days: 46) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 84.98 | 194. | -8.3 | -22.1 | 60.6 | 64.5 |
| Near the Head of Lethe Vallis: PSP_009056_1840 PSP_009900_1840 (Interval in Earth days: 65) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.802 | 153. | 6.66 | -22.9 | 52.4 | 55.9 |
| Hematite in Eos Chasma: PSP_008958_1665 PSP_009380_1665 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.2 | 312. | -4.7 | -21.8 | 63.1 | 64.7 |
| Tyrrhena Terra Crater with Phyllosilicate-Rich Ejecta: PSP_008505_1675 PSP_009085_1675 (Interval in Earth days: 45) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.5 | 83.5 | -9.5 | 14.57 | 61.2 | 61.7 |
| Relatively Deeply Eroded Portion of Marte Vallis: PSP_008567_1985 PSP_008923_1985 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.26 | 185. | 6.87 | -12.2 | 44.4 | 47.1 |
| Textured Plain in Arcadia Planitia: PSP_008566_2285 ESP_016069_2285 (Interval in Earth days: 585) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 48.18 | 209. | -4.0 | -26.0 | 43.4 | 49.7 |
| Athabasca Valles: PSP_009280_1905 PSP_009557_1905 (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 | 10.29 | 156. | 11.7 | -18.0 | 49.3 | 52.2 |
| Tube-Fed Lava Flow Field: PSP_008433_1755 PSP_009501_1755 (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 | -4.58 | 247. | 7.65 | -15.8 | 54.7 | 59.2 |
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