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.
| Subset of Gullies Previously Identified in Dunes in MOC Image M19-01170: PSP_003682_1250 PSP_003748_1250 (Interval in Earth days: 5) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -54.5 | 12.8 | 0.14 | -13.7 | 53.3 | 53.3 |
| South Polar Layered Deposit Comparison with Higher Latitude Scarps: PSP_003868_0940 PSP_003896_0940 (Interval in Earth days: 3) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -85.7 | 13.2 | -0.6 | -19.9 | 67.4 | 70.0 |
| Sublimation Process and Spider Evolution: PSP_003490_0930 PSP_003846_0930 (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 | -86.9 | 274. | 0.41 | 0.79 | 73.5 | 68.7 |
| Cerberus Fossae with Fluvial/Volcanic Features Near Athabasca Vallis Head: PSP_003650_1900 PSP_004283_1900 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 10.01 | 157. | -3.5 | -20.4 | 58.7 | 56.3 |
| Craters with Valley on Both Ends - South End: PSP_003402_1795 PSP_003547_1795 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.40 | 89.6 | -0.6 | 14.47 | 55.1 | 53.4 |
| Light-Toned Layering in Labyrinthus Noctis Pit: PSP_003910_1685 PSP_005400_1685 (Interval in Earth days: 116) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.1 | 261. | 0 | 14.87 | 48.2 | 32.3 |
| Gullies with Tributary Channels in Gorgonum Chaos Crater: PSP_003649_1435 PSP_003794_1435 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -36.3 | 190. | 3.51 | 18.06 | 48.9 | 45.7 |
| Relatively Large Primary Crater on Elysiu Planitia Young Lavas: PSP_003267_1870 PSP_003412_1870 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.153 | 174. | -3.8 | 14.59 | 57.8 | 56.4 |
| Wrinkle Ridge in Elysium Planitia: PSP_003914_1890 PSP_004191_1890 (Interval in Earth days: 22) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.103 | 150. | -3.3 | -29.5 | 57.2 | 57.3 |
| Head of Kasei Valles Cataract: PSP_003948_2055 ESP_039274_2055 (Interval in Earth days: 2752) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 25.01 | 298. | 15.1 | -5.63 | 65.4 | 67.5 |
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