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.
| Sublimation Processes and Spider Evolution : PSP_002652_0930 PSP_002651_0930 (Interval in Earth days: 1) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -86.9 | 96.5 | 7.08 | 22.50 | 87.8 | 86.4 |
| Dark Materials on Block in Olympus Mons Aureole : PSP_002461_1975 ESP_011282_1975 (Interval in Earth days: 687) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.06 | 217. | -4.5 | 16.43 | 56.5 | 56.4 |
| Knobs Near Arrhenius Region : PSP_002478_1365 PSP_003678_1365 (Interval in Earth days: 94) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -42.9 | 120. | 4.1 | -7.1 | 67.2 | 50.4 |
| Ring and Cone Structures Plus Dunes and Other Landforms in Athabasca Valles: PSP_002661_1895 PSP_003294_1895 (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 | 9.569 | 156. | 20.1 | 4.428 | 54.6 | 58.1 |
| Incipient Gullies, As Seen in MOC Image M20-00901: PSP_002146_1335 PSP_002423_1335 (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 | -46.1 | 184. | 6.03 | -15.6 | 72.9 | 70.8 |
| Layered Deposit in an Arabia Region Crater : PSP_002706_1870 PSP_003339_1870 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 6.783 | 10.2 | -4.6 | -19.3 | 56.6 | 59.0 |
| Multiple Episodes of Gully Formation, As Seen in MOC Image R16-02071: PSP_002002_1390 PSP_002846_1390 (Interval in Earth days: 66) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -40.7 | 155. | 8.34 | -14.7 | 71.4 | 62.7 |
| Location of Possible Very Recent Gully Activity: PSP_002040_1435 PSP_002185_1435 (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 | -36.3 | 198. | -3.0 | 11.28 | 69.4 | 67.0 |
| Wrinkle Ridge Cross-Cutting Relationships in Hesperia Planum : PSP_002544_1540 PSP_002689_1540 (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 | -25.8 | 116. | 2.57 | 16.59 | 59.9 | 57.6 |
| Low-Latitude North Polar Layered Deposits and Basal Unit Contact: PSP_001548_2755 PSP_001694_2755 (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 | 84.4 | 142. | 1.30 | 17.73 | 75.0 | 74.8 |
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