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.
| Scalloped Depressions in Amphitrites Patera Region: ESP_033072_1220 ESP_041973_1220 (Interval in Earth days: 694) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -57.6 | 58.7 | 0 | 27.73 | 69.0 | 69.3 |
| Possible Lake Margin in Shalbatana Vallis: ESP_032904_1835 ESP_033537_1835 (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 | 3.523 | 316. | 5.31 | -26.9 | 34.5 | 41.8 |
| Stratigraphic Relation between Gully Aprons and Dunes: ESP_033120_1205 ESP_032896_1205 (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 | -58.9 | 183. | 28.3 | 4.079 | 69.3 | 66.7 |
| Channels and Circular Depression in Phison Rupes Region: ESP_033296_2065 ESP_033586_2065 (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 | 26.21 | 51.5 | -6.6 | 18.33 | 40.1 | 37.7 |
| Deep Crevasses in Glacier-Like Form: ESP_032978_1390 ESP_033400_1390 (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 | -40.8 | 102. | -5.3 | -23.2 | 55.1 | 63.2 |
| Fresh 2-Kilometer Diameter Impact Crater: ESP_033212_1455 ESP_041032_1455 (Interval in Earth days: 609) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -34.0 | 192. | -0.6 | -19.5 | 54.0 | 41.2 |
| Crater with Exposed Layered Walls Superposed on Ejecta of Larger Crater: ESP_033067_1580 ESP_059559_1580 (Interval in Earth days: 2064) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -21.7 | 188. | 6.07 | 22.04 | 43.7 | 41.7 |
| Possible Terraced Crater in Arcadia Planitia: ESP_033053_2245 ESP_033330_2245 (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 | 43.95 | 202. | 5.36 | -17.6 | 50.1 | 49.1 |
| Possible Terraced Bullseye-Like Crater in Arcadia Planitia: ESP_033172_2265 ESP_033594_2265 (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 | 46.20 | 193. | -2.1 | -13.6 | 50.8 | 48.0 |
| Light-Toned Layered Deposits Exposed along Coprates Chasma Floor: ESP_032931_1645 ESP_040975_1645 (Interval in Earth days: 627) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.4 | 302. | -8.6 | 15.73 | 39.8 | 32.4 |
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