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.
| Layers in Terby Crater: PSP_001596_1525 PSP_002216_1525 (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 | -27.3 | 74.2 | 0.12 | -26.4 | 67.8 | 65.5 |
| MSL Landing Site in Melas Chasma: PSP_002828_1700 ESP_019508_1700 (Interval in Earth days: 1300) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.82 | 283. | -28. | -5.16 | 58.0 | 58.0 |
| Inverted Channels near Juventae Chasma: PSP_003223_1755 PSP_003724_1755 (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 | -4.31 | 296. | 0 | 27.52 | 54.6 | 50.0 |
| Southern Layered Mound and Floor in Gale Crater: PSP_002464_1745 PSP_003176_1745 (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 | -5.51 | 138. | 2.93 | 21.29 | 55.7 | 52.8 |
| Central Uplift of Ritchey Crater : PSP_002682_1510 ESP_011635_1510 (Interval in Earth days: 698) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -28.5 | 309. | 5.53 | -13.8 | 59.3 | 61.0 |
| Proposed Strandline: PSP_001820_1985 PSP_003442_1985 (Interval in Earth days: 126) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.25 | 77.3 | 1.02 | -22.9 | 51.3 | 64.1 |
| Layers Exposed in Crater Near Mawrth Vallis: PSP_004052_2045 ESP_012873_2045 (Interval in Earth days: 687) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.30 | 340. | 0 | 15.95 | 65.6 | 65.6 |
| Bright, Fine Layers in Juventae Chasma: PSP_003790_1755 PSP_004291_1755 (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 | -4.61 | 296. | 4.21 | 28.89 | 51.2 | 44.7 |
| Interior Layered Deposits in Candor Chasma : PSP_002696_1745 PSP_003197_1745 (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 | -5.69 | 284. | 0.15 | 26.47 | 55.7 | 52.3 |
| High Thermal-Inertia Terrace Blocks in Holden Crater: PSP_005134_1545 PSP_005978_1545 (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 | -25.4 | 327. | 0 | -26.7 | 33.4 | 39.9 |
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