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.
Reticulate Bedform Change Detection West of Arsia Mons: ESP_022648_1735 ESP_022503_1735 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.30 | 235. | 19.6 | 0.712 | 35.4 | 38.3 |
Gullies and Lobate Material in a Crater in Nereidum Montes: ESP_022540_1405 ESP_023173_1405 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.0 | 308. | 3.88 | -14.2 | 35.4 | 39.5 |
Terra Cimmeria Highland Region: ESP_022321_1470 ESP_065982_1470 (Interval in Earth days: 3402) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -32.8 | 166. | 6.54 | -8.35 | 34.8 | 44.2 |
Bedrock Exposures in Nirgal Vallis: ESP_022645_1505 ESP_023067_1505 (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 | -29.3 | 321. | -3.5 | -19.9 | 33.3 | 34.9 |
Matara Crater Large Dune Gully: ESP_022392_1300 ESP_022115_1300 (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 | -49.5 | 34.8 | -26. | -4.55 | 42.2 | 41.6 |
Coprates Chasma Dune Changes: ESP_022369_1685 ESP_023002_1685 (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 | -11.4 | 293. | 4.01 | -17.8 | 37.5 | 33.6 |
Layered Material in Crater Seen in CTX Image: ESP_022425_1925 ESP_058609_1925 (Interval in Earth days: 2820) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 12.54 | 202. | -5.4 | 8.895 | 50.6 | 37.5 |
Possible Rafted Lava Crust in Tartarus Colles: ESP_022320_2050 ESP_023032_2050 (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 | 24.52 | 188. | -13. | 0.88 | 61.0 | 51.0 |
Central Uplift of Impact Crater: ESP_022454_1470 ESP_022599_1470 (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 | -32.5 | 136. | -0.5 | 16.53 | 34.4 | 32.5 |
Aonia Terra Dune Field Changes: ESP_022488_1300 ESP_022422_1300 (Interval in Earth days: 5) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -49.8 | 293. | -19. | -5.14 | 41.7 | 40.7 |
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