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.
| Stratigraphy Exposed in Ius Chasma: PSP_007430_1725 PSP_009645_1725 (Interval in Earth days: 173) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.24 | 276. | -2.2 | -22.0 | 48.2 | 61.2 |
| Eroded Sediments in West Candor Chasma: PSP_009460_1745 ESP_017741_1745 (Interval in Earth days: 645) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.49 | 284. | 18.2 | 6.762 | 57.4 | 56.6 |
| Unnamed, Well-Preserved Crater South of Hypanis Valles: PSP_009393_1890 PSP_010105_1890 (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 | 8.973 | 313. | -3.9 | 13.87 | 51.3 | 51.3 |
| Dark Spot Near Olmpus Mons Volcano: PSP_009502_1980 ESP_015950_1980 (Interval in Earth days: 503) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.62 | 216. | -2.0 | 26.27 | 48.1 | 36.5 |
| Water Bearing Minerals in Noctis Labyrinthus: PSP_009474_1705 PSP_010107_1705 (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 | -9.28 | 263. | -0.3 | -20.5 | 60.9 | 61.8 |
| Polar Sand Dunes: PSP_008968_2650 PSP_009272_2650 (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 | 84.68 | 0.76 | 0.01 | -16.9 | 59.8 | 61.2 |
| 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 |
| Light Toned Materials and Plains in South Meridiani (MSL): PSP_009563_1770 PSP_009708_1770 (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 | -3.06 | 354. | -15. | 0.701 | 58.4 | 57.3 |
| Landslide Deposits Overlapping the Middle Mount of Coprates Chasma: PSP_008616_1685 PSP_009051_1685 (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 | -11.5 | 291. | -2.7 | 14.75 | 60.6 | 60.9 |
| Central Peak of Large Well-Preserved Crater: PSP_008860_2165 ESP_053799_2160 (Interval in Earth days: 3502) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.93 | 101. | 5.76 | -5.62 | 41.8 | 42.8 |
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