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.
Saheki Crater Alluvial Fan Layering Exposed in Eastern Portion of Crater: ESP_012949_1580 ESP_013226_1580 (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 | -21.7 | 73.0 | 0.82 | -26.3 | 44.2 | 42.9 |
Fresh Central Pit Crater in Southern Highlands: ESP_012727_1540 ESP_013149_1540 (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 | -25.8 | 14.6 | -3.1 | -14.1 | 46.9 | 42.2 |
Gully and Fan in Southern Hemisphere Crater: ESP_013478_1300 ESP_021614_1300 (Interval in Earth days: 634) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -49.5 | 34.8 | -1.1 | -21.7 | 41.9 | 48.2 |
Possible Sulfates in Ius Chasma: ESP_013759_1720 ESP_020550_1720 (Interval in Earth days: 529) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.88 | 276. | 4.68 | -17.6 | 38.5 | 55.9 |
Fretted Terrain-Like Aprons Near Reull Vallis: ESP_012935_1415 ESP_013212_1415 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.2 | 96.9 | 6.90 | -17.4 | 43.4 | 41.9 |
Light-Toned Fan-Like Features in Crater in Chryse Chaos: ESP_013256_1885 ESP_022104_1885 (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 | 8.534 | 327. | -1.4 | -13.8 | 53.6 | 52.2 |
Channel Carved Into Scarp within Isidis Planitia: ESP_013186_1945 ESP_013252_1945 (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 | 14.55 | 78.4 | -2.7 | -24.1 | 58.1 | 58.9 |
Fluidized Ejecta in the Kasei Valles Region: ESP_013204_2060 ESP_083253_2060 (Interval in Earth days: 5458) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 25.76 | 305. | 0 | 16.06 | 65.4 | 67.6 |
A Fan in a Southern Highlands Crater: ESP_014159_1670 ESP_020106_1670 (Interval in Earth days: 464) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.7 | 157. | -7.0 | 7.119 | 34.6 | 56.0 |
Possible Rootless Cones in Hydraotes Chaos: ESP_013177_1800 ESP_021458_1800 (Interval in Earth days: 645) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.053 | 326. | -4.9 | -21.2 | 49.8 | 53.9 |
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