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.
| Possible Collapsed Slab Along Walls of Mamers Vallis: PSP_003510_2165 PSP_003576_2165 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.28 | 15.3 | 8.84 | -8.55 | 71.8 | 73.4 |
| Seasonal Sublimation Process / Spider Evolution: PSP_003219_0930 PSP_003220_0930 (Interval in Earth days: 0) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -86.9 | 100. | 6.01 | -4.11 | 77.4 | 78.6 |
| Relatively Dust Free Lavas from Arsia Mons: PSP_003160_1410 ESP_047413_1410 (Interval in Earth days: 3448) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.8 | 220. | 2.16 | 26.86 | 56.5 | 49.2 |
| Possible Small Volcano at Syria Planum: PSP_004187_1675 ESP_056787_1675 (Interval in Earth days: 4099) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.3 | 261. | -26. | -5.64 | 46.8 | 45.7 |
| Light-Toned Layers in Crater South of Crommelin Crater: PSP_003788_1820 ESP_020679_1820 (Interval in Earth days: 1316) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.194 | 351. | 0 | 13.94 | 54.3 | 54.3 |
| Square-Shaped Fresh Crater Near Gratteri Crater: PSP_004044_1640 PSP_004110_1640 (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 | -15.7 | 203. | 5.46 | -17.2 | 45.1 | 46.0 |
| Light Material in Ius Chasma: PSP_003949_1725 PSP_004305_1725 (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 | -7.23 | 276. | 0 | 11.10 | 49.2 | 44.8 |
| Odd Layered and Eroding Crater Fill in Deeply Eroded Craters: PSP_003773_1630 PSP_003918_1630 (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 | -16.8 | 42.7 | 1.82 | 18.06 | 48.1 | 45.3 |
| Crater with Unusual Yet Original Morphology: PSP_003964_1910 PSP_004241_1910 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 10.63 | 224. | 2.57 | -24.2 | 57.4 | 57.3 |
| Fresh Crater: PSP_003942_1585 ESP_058138_1585 (Interval in Earth days: 4223) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -21.1 | 109. | 1.8 | -11.9 | 45.4 | 31.0 |
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