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.
Northern Spring Monitor Site with Known Multi-Toned Defrost Spots: PSP_009249_2650 PSP_009342_2650 (Interval in Earth days: 7) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 84.94 | 234. | 8.69 | -5.93 | 60.1 | 60.9 |
Very Fresh Unnamed 10-Kilometer Peak Pit Crater in Utopia Planitia: PSP_009098_2140 PSP_009164_2140 (Interval in Earth days: 5) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 33.47 | 84.1 | -3.1 | -20.4 | 43.4 | 45.2 |
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 |
Abrading Dome Dunes in the North Polar Erg: PSP_009295_2565 PSP_009743_2565 (Interval in Earth days: 35) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 76.17 | 95.3 | -6.2 | 15.45 | 55.6 | 56.7 |
Isolated Gully at Intersection of Wrinkle Ridge and Crater Wall: PSP_008608_1510 PSP_009043_1510 (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 | -28.8 | 152. | -8.0 | 7.793 | 72.7 | 73.1 |
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 |
Smooth Crater Floor with Bounding Terrace on Flank of Uranius Mons: PSP_008788_2065 PSP_009355_2065 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 26.42 | 268. | 8.34 | -5.68 | 42.7 | 45.5 |
Crater with Impressive Wind Streak in Elysium Planitia: PSP_008304_1860 ESP_012919_1860 (Interval in Earth days: 360) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 5.728 | 169. | -2.0 | -11.4 | 49.1 | 55.9 |
Well-Preserved 9-Kilometer Diameter Crater: PSP_008902_1565 PSP_009680_1565 (Interval in Earth days: 60) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -23.0 | 43.1 | -5.5 | -19.4 | 69.6 | 70.5 |
Chain of Mounds in the Tharsis Region: PSP_008262_1855 ESP_042652_1855 (Interval in Earth days: 2679) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 5.645 | 237. | -7.4 | -23.4 | 49.3 | 43.3 |
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