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.
Sharp-Looking Gullies : PSP_002888_1400 PSP_004167_1400 (Interval in Earth days: 100) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.6 | 87.9 | -8.1 | 14.24 | 61.4 | 41.4 |
Pit Crater Chains and Cross-Cutting Graben in Tractus Catena: PSP_002064_2025 PSP_002776_2025 (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 | 22.18 | 255. | -6.8 | 9.417 | 53.9 | 59.1 |
Gullies Possibly Produced by Snow/Ice Melting : PSP_003096_1375 PSP_003940_1375 (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 | -42.2 | 169. | -6.1 | -22.4 | 59.0 | 47.6 |
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 |
Chasma Boreale Scarp with Possible Gypsum: PSP_001374_2650 PSP_001518_2650 (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 | 85.02 | 338. | -7.1 | 13.56 | 67.8 | 68.9 |
Lineated Valley Fill in Coloe Fossae : PSP_002902_2205 PSP_003245_2205 (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 | 40.17 | 53.8 | 3.42 | -28.6 | 68.0 | 74.6 |
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 |
Fractured Mounds at the Southern Edge of Elysium Planitia : PSP_002542_1765 PSP_003597_1765 (Interval in Earth days: 82) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.25 | 167. | 8.70 | -21.0 | 55.0 | 54.9 |
Crater and Extensive Field of Secondary Craters Seen in MOC Image R15-02146: PSP_002230_1850 ESP_027890_1850 (Interval in Earth days: 1999) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.727 | 46.1 | -7.8 | 4.118 | 55.2 | 51.4 |
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 |
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