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.
| Channel Bedforms and Fan North of Arabia Terra: ESP_068533_2195 ESP_078173_2195 (Interval in Earth days: 751) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 39.35 | 33.9 | 4.61 | -7.92 | 50.5 | 44.5 |
| Impact Crater adjacent to Ravine: ESP_068867_1985 ESP_078823_1985 (Interval in Earth days: 776) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.09 | 288. | 1.03 | 12.18 | 45.8 | 44.6 |
| Modification of Small Terraced Crater: ESP_068829_2480 ESP_069251_2480 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 67.82 | 233. | 4.32 | 25.32 | 62.9 | 57.0 |
| Very Well-Preserved 900-Meter Northern Plains Crater : ESP_068700_2420 ESP_068687_2420 (Interval in Earth days: 1) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 61.49 | 155. | -0.2 | -26.2 | 60.9 | 63.1 |
| Cones in Tharsis Region: ESP_068895_1890 ESP_069093_1890 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.120 | 243. | 26.6 | 2.819 | 44.7 | 48.4 |
| Crater Gullies at Multiple Elevations: ESP_067299_1435 ESP_067708_1435 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -36.1 | 227. | -6.6 | 3.913 | 42.9 | 47.4 |
| Layered Deposits on South Wall of West Candor Chasma: ESP_068392_1730 ESP_076832_1730 (Interval in Earth days: 658) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.96 | 284. | 21.9 | 0.965 | 43.9 | 37.3 |
| Eos Chasma Slumps: ESP_068444_1630 ESP_067718_1630 (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 | -16.6 | 310. | -18. | 14.65 | 51.0 | 39.5 |
| Streamlined Form in Kasei Valles: ESP_068326_1990 ESP_069474_1990 (Interval in Earth days: 89) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.78 | 283. | -7.8 | 6.899 | 45.0 | 48.4 |
| Modified Fan in Shalbatana Vallis: ESP_068457_1760 ESP_078598_1760 (Interval in Earth days: 790) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.18 | 313. | -0.6 | 22.00 | 45.7 | 52.6 |
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