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.
| Small Crater: ESP_032935_2290 ESP_033001_2290 (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 | 48.57 | 183. | 7.56 | -7.53 | 54.5 | 54.6 |
| Possible Terraced Bullseye-Like Crater in Arcadia Planitia: ESP_033132_2205 ESP_033211_2205 (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 | 39.95 | 206. | 2.77 | 26.56 | 47.0 | 44.5 |
| Fan in Trough in Aeolis Region in CTX Image: ESP_033174_1735 ESP_042919_1735 (Interval in Earth days: 759) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.20 | 145. | 5.64 | 15.90 | 38.2 | 47.6 |
| Candidate New Impact Site Formed between January 2008 and July 2012: ESP_033237_1855 ESP_033738_1855 (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 | 5.640 | 224. | 3.15 | 23.75 | 36.5 | 38.7 |
| Possible Fissure Volcano in Syria Planum: ESP_033038_1675 ESP_033315_1675 (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 | -12.6 | 259. | 8.43 | -27.7 | 38.8 | 45.0 |
| Possible Terraced Crater in Arcadia Planitia: ESP_033277_2210 ESP_033554_2210 (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 | 40.85 | 207. | 1.29 | -20.4 | 46.4 | 46.1 |
| Hydrated Minerals along Coprates Chasma Wallrock: ESP_033010_1645 ESP_033788_1645 (Interval in Earth days: 61) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.2 | 303. | 18.7 | 5.278 | 38.7 | 50.3 |
| Light-Toned Layered Deposits at Contact between Ladon Valles and Basin: ESP_032930_1595 ESP_032864_1595 (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 | -20.2 | 329. | -1.9 | 22.16 | 41.4 | 38.7 |
| Floor of East Candor Chasma: ESP_033274_1725 ESP_033419_1725 (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 | -7.64 | 295. | 1.74 | 15.84 | 40.2 | 40.9 |
| Western Rim of Well-Preserved Impact Crater in Tyrrhena Terra: ESP_033189_1615 ESP_042011_1615 (Interval in Earth days: 688) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -18.5 | 98.4 | -7.3 | 8.201 | 44.6 | 44.5 |
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