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.
Gullies: PSP_007456_2140 ESP_016040_2140 (Interval in Earth days: 669) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 33.74 | 281. | -4.6 | -22.7 | 41.7 | 43.6 |
Unnamed Small Rayed Crater in Hesperia Region: PSP_008135_1520 PSP_008425_1520 (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 | -27.9 | 108. | -4.0 | 6.037 | 68.6 | 70.2 |
Putative Salt Deposits Detected by THEMIS West of Meridiani Region: PSP_007981_1770 PSP_008851_1770 (Interval in Earth days: 68) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.06 | 350. | -5.6 | 23.21 | 51.6 | 54.5 |
Small Channel in Elysium Planitia: PSP_008265_1860 PSP_008990_1860 (Interval in Earth days: 57) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 5.981 | 155. | -6.8 | 12.22 | 49.1 | 50.7 |
Proposed MSL Landing Site in Holden Crater: PSP_008193_1535 PSP_008483_1535 (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 | -26.1 | 325. | -7.5 | 0.702 | 68.1 | 69.7 |
Proposed MSL Landing Site in Mawrth Vallis - Ellipse 4: PSP_008390_2050 PSP_008891_2050 (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 | 24.79 | 339. | -7.3 | -21.7 | 43.3 | 46.0 |
Wrinkle Ridges in Western Elysium Planitia: PSP_007896_1890 PSP_009689_1890 (Interval in Earth days: 140) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.738 | 150. | -7.9 | 13.26 | 45.7 | 50.7 |
Channel into Jezero Crater Delta: PSP_007925_1990 PSP_008650_1990 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.85 | 77.5 | -7.4 | 17.24 | 42.8 | 43.6 |
Ridges in Huo Hsing Vallis : PSP_008189_2080 PSP_007833_2080 (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 | 27.52 | 67.0 | -1.3 | 7.894 | 41.8 | 40.2 |
Well Preserved Impact Crater of Alba Patera: PSP_006745_2250 PSP_007035_2250 (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 | 44.64 | 253. | 2.65 | 17.88 | 49.7 | 46.1 |
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