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.
| 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 |
| Strike-Slip Fault in Amazonis Planitia: PSP_008540_2020 PSP_009898_2020 (Interval in Earth days: 106) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.90 | 203. | -6.2 | 10.50 | 44.3 | 47.3 |
| 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 |
| 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 |
| Crater in Mawrth Region: PSP_008258_2075 ESP_024978_2075 (Interval in Earth days: 1303) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 27.28 | 342. | 4.71 | -21.4 | 41.5 | 40.5 |
| Gullies on Top of Dunes As Seen in MOC Image M17-01035: PSP_008739_1425 PSP_007592_1425 (Interval in Earth days: 89) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.4 | 176. | -7.2 | 4.827 | 79.4 | 69.0 |
| Cluster of Cones in Utopia Planitia: PSP_008544_2095 PSP_009124_2095 (Interval in Earth days: 45) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 29.12 | 93.0 | -7.1 | 14.61 | 42.9 | 42.5 |
| Merging Lobate Debris Aprons of Deuteronilus Mensae: PSP_008744_2240 PSP_009535_2240 (Interval in Earth days: 62) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 43.76 | 29.3 | -6.2 | 15.83 | 43.0 | 43.5 |
| Channels Emanating from Cerberus Fossae: PSP_008660_1945 PSP_009016_1945 (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 | 14.38 | 166. | 4.34 | -12.1 | 46.4 | 48.8 |
| High-Latitude Exposure of North Polar Layered Deposits: PSP_009187_2680 ESP_018221_2680 (Interval in Earth days: 704) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 87.92 | 95.3 | -6.5 | -14.0 | 63.1 | 63.7 |
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