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.
| Mesas and Buttes of Hydraotes Chaos: ESP_021893_1805 ESP_031163_1805 (Interval in Earth days: 722) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.634 | 327. | 3.40 | 22.57 | 48.7 | 42.4 |
| Well-Preserved 10-Kilometer Diameter Gullied Impact Crater: ESP_021712_1400 ESP_021989_1400 (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 | -39.5 | 234. | 6.62 | -17.0 | 42.3 | 40.7 |
| Bedform Changes in Aureum Chaos: ESP_021906_1765 ESP_022183_1765 (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 | -3.64 | 333. | -1.9 | -28.1 | 46.7 | 45.5 |
| Northern Part of Asimov Crater Ring Trough: ESP_021694_1330 ESP_021760_1330 (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 | -46.4 | 4.90 | 21.1 | 4.178 | 42.9 | 43.4 |
| Sinuous Ridge and Surrounding Material Southwest of Capen Crater: ESP_021654_1855 ESP_030212_1855 (Interval in Earth days: 667) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 5.284 | 12.7 | -2.8 | 9.786 | 53.7 | 54.3 |
| Central Uplift with Layers and Clays: ESP_021688_1325 ESP_021754_1325 (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 | -47.2 | 170. | 2.61 | -14.9 | 44.6 | 45.1 |
| Candidate New Gully Flow Formed between 15 May 2009 and 3 March 2011: ESP_021914_1475 ESP_022336_1475 (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 | -32.3 | 118. | 3.26 | -10.0 | 39.2 | 35.9 |
| Lots of Layers in Terby Crater: ESP_021942_1520 ESP_021797_1520 (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 | -27.6 | 74.7 | -9.8 | -24.5 | 39.9 | 43.0 |
| Folded Layers on Floor of Ius Chasma: ESP_021552_1725 ESP_022185_1725 (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 | -7.48 | 279. | -6.1 | -28.2 | 48.9 | 43.7 |
| Terrain in Promethei Terra: ESP_021466_1230 ESP_021954_1230 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -56.6 | 114. | 1.91 | -20.9 | 51.2 | 47.2 |
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