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.
Concentric Ridges Near Alcoves Northwest of Oudemans Crater: PSP_008986_1715 PSP_009408_1715 (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 | -8.27 | 266. | 8.18 | -9.64 | 59.2 | 60.9 |
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 |
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 |
Smooth Crater Floor with Bounding Terrace on Flank of Uranius Mons: PSP_008788_2065 PSP_009355_2065 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 26.42 | 268. | 8.34 | -5.68 | 42.7 | 45.5 |
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 |
Landslides in Ganges Chasma: PSP_009037_1715 PSP_009538_1715 (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 | -8.54 | 315. | -14. | 7.943 | 60.9 | 59.8 |
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 |
Potential Phyllosilicates in Acidalia Region: PSP_009182_2215 PSP_009472_2215 (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 | 41.28 | 309. | -4.4 | 16.00 | 43.6 | 43.0 |
Possible Gullies in Dunes: PSP_008751_1795 PSP_009186_1795 (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 | -0.40 | 204. | -13. | 14.12 | 55.2 | 54.4 |
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 |
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