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.
Naar Crater: PSP_007046_2030 ESP_025691_2030 (Interval in Earth days: 1453) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 22.90 | 317. | 3.89 | -21.5 | 39.0 | 42.0 |
Small Craters in Amazonis Planitia: PSP_008092_1980 PSP_008527_1980 (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 | 17.87 | 197. | -5.7 | 8.084 | 43.7 | 44.3 |
Small Fresh Primary or Large Secondary Crater From Gratteri Crater: PSP_007209_1565 PSP_008290_1565 (Interval in Earth days: 84) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -23.3 | 194. | -6.7 | 16.15 | 54.8 | 65.4 |
Northwest Hellas Basin Landforms: PSP_007636_1400 ESP_016075_1400 (Interval in Earth days: 658) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.4 | 55.9 | 0.23 | -23.1 | 71.3 | 67.4 |
Central Pit of Large Crater South of Valles Marineris: PSP_007047_1640 PSP_010264_1640 (Interval in Earth days: 251) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.9 | 296. | -7.3 | 5.642 | 48.3 | 63.0 |
Cones and Pitted Material Inside An Embayed Crater in the Tartarus Montes: PSP_007605_2055 PSP_007961_2055 (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 | 25.39 | 173. | 4.99 | -5.25 | 40.0 | 41.8 |
Etched Terrain with Possible Layering West of Juventae Chasma: PSP_007482_1760 PSP_009486_1760 (Interval in Earth days: 156) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.20 | 296. | 1.06 | -9.01 | 47.0 | 58.5 |
Light-Toned Tilted Layering in Central Peak of Oudemans Crater: PSP_007694_1700 ESP_027882_1700 (Interval in Earth days: 1574) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.92 | 268. | 1.09 | -17.4 | 52.3 | 59.3 |
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 |
Gullies on South-Facing Wall of Crater: PSP_007045_1450 ESP_016130_1450 (Interval in Earth days: 708) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -34.6 | 353. | -5.7 | -23.5 | 59.8 | 64.8 |
Page 750 of 840 (8,398 images) |