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.
| Lineated Valley Fill in Coloe Fossae: PSP_008598_2155 PSP_008954_2155 (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 | 35.16 | 57.2 | -3.6 | -18.8 | 42.2 | 44.3 |
| Layers in Uzboi Vallis: PSP_008338_1525 PSP_010329_1525 (Interval in Earth days: 155) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.4 | 324. | 5.23 | -10.4 | 69.3 | 70.2 |
| Crater Floor Fan: PSP_008233_1920 PSP_008879_1920 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 11.72 | 307. | 6.25 | -7.44 | 45.5 | 49.1 |
| Very Recent Small Crater in Dejnev Crater: PSP_008145_1545 ESP_027067_1545 (Interval in Earth days: 1474) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -25.0 | 195. | -8.7 | 6.238 | 66.9 | 69.0 |
| Inner Channel Deposit in Kasei Vallis: PSP_007825_2010 ESP_035463_2010 (Interval in Earth days: 2153) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 20.84 | 287. | -3.9 | 12.13 | 41.7 | 43.8 |
| Topographically-Deflected Ejecta in Chryse Planitia: PSP_007916_2010 ESP_016078_2010 (Interval in Earth days: 636) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 20.91 | 322. | 0.50 | 15.41 | 41.8 | 38.0 |
| Flow-Banded Deformed Terrain of Hellas Basin Floor: PSP_007201_1405 PSP_007491_1405 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.9 | 54.9 | -7.0 | 3.906 | 65.3 | 68.9 |
| Upper Section of Northern Olympus Mons Basal Scarp: PSP_007445_2035 PSP_008447_2035 (Interval in Earth days: 78) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 22.90 | 223. | -1.4 | -13.8 | 40.1 | 44.4 |
| 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 |
| Light Outcrop in Aurorae Chaos: PSP_007705_1730 PSP_009498_1730 (Interval in Earth days: 140) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.78 | 327. | -5.9 | 5.161 | 51.2 | 59.1 |
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