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.
Exposure of North Polar Layered Deposits: ESP_019343_2685 ESP_028008_2685 (Interval in Earth days: 675) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 88.28 | 50.8 | -14. | -24.3 | 74.8 | 73.1 |
Alpine Glacier: ESP_019213_2210 ESP_019503_2210 (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 | 40.86 | 51.3 | -8.0 | 14.46 | 51.2 | 52.7 |
Translucent Ice on Dunes: ESP_019006_2550 ESP_019243_2550 (Interval in Earth days: 18) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 74.97 | 300. | -21. | 3.245 | 63.1 | 64.3 |
Gullies in Wall of Smaller Crater within Arrhenius Crater: ESP_018947_1400 ESP_019369_1400 (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 | -39.6 | 123. | 1.96 | -11.3 | 77.1 | 74.5 |
High-Latitude Exposure of North Polar Layered Deposits: ESP_019117_2720 ESP_019050_2720 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 87.74 | 6.00 | -13. | -23.1 | 73.5 | 73.7 |
Steep North Polar Boundary Scarp: ESP_018943_2655 ESP_019181_2655 (Interval in Earth days: 19) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 85.36 | 186. | 0 | -13.2 | 67.0 | 70.6 |
Well-Preserved Impact Crater in Arabia Terra: ESP_019162_1975 ESP_019439_1975 (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 | 17.23 | 5.48 | 7.48 | -19.6 | 48.9 | 52.7 |
Possible Crater: ESP_019164_1705 ESP_035093_1705 (Interval in Earth days: 1241) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.50 | 314. | 2.70 | -7.72 | 58.2 | 59.2 |
Impact Crater with Central Uplift: ESP_019059_1490 ESP_027894_1490 (Interval in Earth days: 689) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -30.7 | 303. | 8.37 | -18.5 | 70.2 | 71.1 |
Possible MSL Rover Landing Site Holden Crater: ESP_019045_1530 ESP_019322_1530 (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 | -26.6 | 325. | 8.87 | -19.8 | 67.8 | 68.0 |
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