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.
| Rayed Crater: PSP_001660_1950 PSP_002570_1950 (Interval in Earth days: 71) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 14.87 | 123. | -1.8 | -15.8 | 51.0 | 57.9 |
| Layered Deposits with Proposed Cross-Bedding: PSP_002023_1755 PSP_002379_1755 (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 | -4.37 | 297. | 2.82 | 12.63 | 55.8 | 54.9 |
| Layering in Danielson Crater : PSP_002944_1880 ESP_019835_1880 (Interval in Earth days: 1317) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.951 | 352. | -11. | 10.60 | 58.1 | 52.8 |
| 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 |
| Dark-Toned Unit Exposed atop Crater Ejecta in Meridiani Planum : PSP_002680_1825 PSP_003392_1825 (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 | 2.240 | -0.3 | 7.78 | 29.45 | 55.2 | 53.5 |
| Contact Between Layering in Plains and Wallrock Near Ius Chasma : PSP_002459_1715 PSP_003092_1715 (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 | -8.30 | 275. | -0.0 | -21.4 | 56.4 | 56.3 |
| Gullies on Very High Dune Slip Face in Russell Crater: PSP_001440_1255 PSP_001981_1255 (Interval in Earth days: 42) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -54.2 | 12.9 | 8.51 | -8.06 | 85.6 | 80.5 |
| Low Shield with Elongate Summit Depression in North Tharsis Region : PSP_002328_2080 PSP_002605_2080 (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 | 27.56 | 246. | 2.86 | -21.7 | 56.5 | 61.5 |
| Light-Toned Dome on Northern Plains: PSP_002233_2225 PSP_002866_2225 (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 | 42.13 | 319. | -5.7 | -19.4 | 60.0 | 70.3 |
| Lobate Debris Apron with Ridge-Like Structures; Tempe Terra/Mareotis Fossae: PSP_002590_2320 PSP_003078_2320 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 51.77 | 289. | 7.55 | -12.9 | 68.4 | 77.6 |
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