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.
| Gullies: ESP_032989_1435 ESP_067209_1435 (Interval in Earth days: 2666) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -36.3 | 161. | -5.2 | 6.212 | 52.1 | 41.1 |
| Possible Fossil Dunes in Noachis Terra: ESP_032941_1310 ESP_033020_1310 (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 | -48.9 | 34.0 | -2.6 | 22.11 | 60.1 | 60.2 |
| Candidate New Impact Site Formed between December 2011 and December 2012: ESP_033093_1605 ESP_059506_1605 (Interval in Earth days: 2058) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -19.3 | 198. | 5.11 | -15.9 | 42.8 | 42.1 |
| Ridges in Meridiani Planum: ESP_033206_1800 ESP_033496_1800 (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 | 0.069 | 351. | 0.89 | 27.28 | 37.3 | 37.8 |
| Crater with Trough: ESP_032965_2315 ESP_033809_2315 (Interval in Earth days: 65) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 51.06 | 84.6 | -2.2 | -22.5 | 56.4 | 49.7 |
| Central Peak of Taxco Crater: ESP_033273_2010 ESP_042095_2010 (Interval in Earth days: 687) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 20.64 | 319. | -3.3 | 11.76 | 38.3 | 37.9 |
| Enigmatic Channels on the Floor of Mangala Valles: ESP_033053_1640 ESP_033264_1640 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.6 | 210. | 2.12 | -10.2 | 40.7 | 44.4 |
| Pedestal Crater in Arcadia Planitia: ESP_032921_2355 ESP_033145_2355 (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 | 55.13 | 204. | -0.0 | 22.74 | 59.9 | 55.7 |
| Well-Preserved Impact Crater with Steep Slopes: ESP_032975_1415 ESP_033041_1415 (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 | -38.2 | 183. | -4.1 | -24.0 | 53.1 | 55.4 |
| Floor of East Candor Chasma: ESP_032918_1720 ESP_032984_1720 (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 | -7.80 | 295. | 6.17 | -19.3 | 35.9 | 38.6 |
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