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.
| Dry Cataract North of Mangala Valles: PSP_008909_1805 PSP_009120_1805 (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 | 0.327 | 208. | 4.84 | -8.79 | 54.0 | 55.5 |
| Central Peak of Well-Preserved Crater Northwest of Tartarus Montes: PSP_009240_2055 ESP_017943_2055 (Interval in Earth days: 678) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 25.01 | 167. | 6.15 | -17.6 | 44.5 | 45.1 |
| Recent Impact Crater in the Phlegra Dorsa and Tartarus Montes Regions: PSP_009121_2005 ESP_019314_2005 (Interval in Earth days: 794) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 20.31 | 177. | 4.14 | -15.3 | 45.6 | 51.3 |
| 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 |
| Ganges Catena Pit Crater Chain Cut by Wrinkle Ridge: PSP_008326_1775 PSP_008827_1775 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.33 | 289. | 5.91 | -12.9 | 52.9 | 56.5 |
| Lineated Valley Fill in Coloe Fossae: PSP_008743_2155 PSP_009033_2155 (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 | 35.34 | 57.0 | 1.58 | 10.94 | 42.0 | 41.8 |
| Field of Cones in the Tartarus Montes: PSP_008528_2060 PSP_009675_2060 (Interval in Earth days: 90) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 25.80 | 170. | -7.7 | 13.02 | 43.5 | 45.3 |
| Seasonal Frost on Dunes: PSP_008847_2580 PSP_009256_2580 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 77.98 | 84.0 | -2.5 | -17.7 | 55.7 | 57.3 |
| Dissected Terraces of an Unnamed Crater: PSP_008327_1995 PSP_009263_1995 (Interval in Earth days: 73) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 19.27 | 260. | -6.4 | 8.129 | 44.3 | 46.0 |
| Gullies: PSP_008984_2135 ESP_017476_2135 (Interval in Earth days: 662) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 33.30 | 315. | 3.85 | -10.4 | 42.5 | 42.3 |
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