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.
| Gully-Like Features on Dunes in MOC Image R10-03153: ESP_014067_1150 ESP_021583_1150 (Interval in Earth days: 586) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -64.5 | 158. | -5.6 | 20.41 | 53.4 | 51.9 |
| Layers on Columbus Crater Wall: ESP_014105_1495 ESP_014382_1495 (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 | -30.0 | 193. | -0.6 | -23.8 | 34.9 | 38.0 |
| Geologic Contact North of Arabia Terra: ESP_014138_2235 ESP_022643_2235 (Interval in Earth days: 662) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 43.14 | 3.39 | -2.8 | 24.50 | 67.8 | 69.9 |
| Alcove in East Candor Chasma Layered Deposits: ESP_012809_1725 ESP_013310_1725 (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 | -7.44 | 293. | -2.1 | 22.37 | 50.2 | 42.7 |
| Fretted Terrain-Like Aprons Near Reull Vallis: ESP_013001_1415 ESP_013146_1415 (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 | -38.4 | 97.3 | -15. | -1.78 | 44.3 | 41.5 |
| Possible Blocky Deposit in Melas Chasma: ESP_013508_1665 ESP_014141_1665 (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 | -13.2 | 289. | 6.08 | -18.0 | 39.2 | 35.6 |
| Exposure of Layered Sequence in Terby Crater: ESP_013160_1530 ESP_074031_1530 (Interval in Earth days: 4743) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -26.9 | 74.0 | -8.4 | 2.702 | 41.5 | 52.0 |
| Impact Crater with a Rocky Central Uplift: ESP_012947_1735 ESP_022441_1735 (Interval in Earth days: 740) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.55 | 125. | 4.88 | 27.14 | 48.6 | 37.0 |
| Basal Exposure of South Polar Layered Deposits: ESP_013857_1070 ESP_014015_1070 (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 | -72.6 | 135. | -5.1 | 19.52 | 57.3 | 57.5 |
| Stratigraphic Relations in THEMIS Image V11134006 in Sinus Meridiani: ESP_013703_1800 ESP_021984_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 | -0.14 | 2.99 | 25.0 | 10.04 | 41.4 | 46.9 |
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