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.
| Light-Toned Layered Bedrock Exposed in Valles Marineris : PSP_002722_1665 PSP_003355_1665 (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 | -13.1 | 295. | 2.08 | -13.4 | 56.1 | 53.6 |
| Light-Toned Layering in Plains South of Melas Chasma : PSP_002617_1690 PSP_003118_1690 (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 | -11.0 | 281. | -0.7 | 24.63 | 56.4 | 52.2 |
| Eroded Layers and Scallops and Polygons: PSP_001964_2275 PSP_003177_2275 (Interval in Earth days: 95) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 46.94 | 101. | -0.2 | 25.63 | 57.4 | 73.6 |
| 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 |
| Gully Orientation Survey: PSP_001823_1320 PSP_001691_1320 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -47.4 | 4.36 | -0.8 | 13.07 | 78.0 | 78.5 |
| 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 | 59.2 |
| Central Uplift of an Impact Crater: PSP_002353_1585 PSP_003408_1585 (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 | -21.4 | 290. | 0 | -26.3 | 60.2 | 53.6 |
| Layered Deposit in a Small Crater within Schiaparelli Crater: PSP_002363_1800 PSP_002508_1800 (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 | -0.18 | 14.4 | 7.82 | 23.78 | 54.7 | 53.5 |
| Channels South of the Base of Ascraeus Mons: PSP_001985_1860 PSP_002486_1860 (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 | 5.998 | 254. | -3.9 | 22.18 | 54.0 | 53.5 |
| Northern Plains Sample: PSP_001945_2515 PSP_002077_2515 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 71.07 | 252. | 2.20 | -10.6 | 67.4 | 70.6 |
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