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.
| Vertical Exposure of Layering in West Candor Chasma: PSP_007021_1740 PSP_007232_1740 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.82 | 283. | 5.28 | -9.86 | 42.3 | 45.8 |
| Landslide Scarp: PSP_007785_1645 PSP_008141_1645 (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 | -15.1 | 303. | 7.47 | -3.79 | 56.0 | 60.0 |
| Dark Dune-Like Forms in Southern Melas Chasma: PSP_007522_1685 ESP_025666_1685 (Interval in Earth days: 1414) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.1 | 284. | 0.94 | -27.7 | 51.1 | 56.6 |
| Bright Gully Fans: PSP_007429_2440 PSP_008141_2440 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 63.78 | 292. | 2.14 | -7.16 | 55.0 | 50.5 |
| Faults in Ius Chasma: PSP_008010_1720 PSP_009658_1720 (Interval in Earth days: 129) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.82 | 279. | -4.9 | 7.572 | 54.5 | 59.5 |
| Layers and Scallops: PSP_007252_2265 PSP_007687_2265 (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 | 46.28 | 90.9 | -7.8 | 5.11 | 47.3 | 44.0 |
| Middle Section of Northern Olympus Mons Basal Scarp: PSP_007089_2035 PSP_007946_2035 (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 | 23.25 | 223. | 7.43 | -6.64 | 38.8 | 42.1 |
| Line of Cones and Associated Flows in Arsia Sulci: PSP_007603_1770 ESP_036718_1770 (Interval in Earth days: 2269) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.83 | 231. | 8.18 | -17.6 | 47.1 | 57.8 |
| Layered Bedrock Exposed in Central Uplift of Crater in Thaumasia Planum: PSP_007113_1595 PSP_007469_1595 (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 | -20.3 | 293. | 4.00 | -7.61 | 50.9 | 56.5 |
| Light-Toned Layered Deposits Along Plains South of Ius Chasma: PSP_007786_1710 PSP_009935_1710 (Interval in Earth days: 167) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.74 | 276. | -4.8 | 20.55 | 52.9 | 58.8 |
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