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.
| Ridge in Hadriacus Patera: ESP_092860_1490 ESP_093071_1490 (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 | -30.6 | 92.8 | 7.43 | -5.39 | 36.8 | 36.4 |
| Cryptic Terrain Margin Monitoring near Promethei Rupes: ESP_092862_1000 ESP_093165_1000 (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 | -79.6 | 55.5 | 0.32 | 17.08 | 60.1 | 61.1 |
| Possible Compound Dune in USGS Dune Database Entry Number 1161-770: ESP_092741_1030 ESP_093466_1030 (Interval in Earth days: 57) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -77.0 | 116. | 1.75 | 17.03 | 57.9 | 62.5 |
| Irregular Cellular Structures on Crater Floor South of Corozal Crater: ESP_093029_1365 ESP_092950_1365 (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 | -43.1 | 159. | 9.10 | -19.1 | 38.5 | 40.7 |
| Terrain Sample in Candidate Future Landing Site: ESP_092859_2090 ESP_093347_2090 (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 | 28.64 | 110. | 23.5 | -8.99 | 63.6 | 59.3 |
| Light-Toned Layered Deposits on Northern Edge of Hellas Planitia: ESP_092927_1530 ESP_093428_1530 (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 | -26.8 | 62.9 | 7.73 | 28.36 | 36.2 | 32.5 |
| Fluvial Channel in Nirgal Vallis: ESP_093010_1520 ESP_092865_1520 (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 | -27.5 | 316. | 5.82 | -4.21 | 35.7 | 37.5 |
| Volcanic Cone and Lava Flow: ESP_092978_2050 ESP_093123_2050 (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 | 24.75 | 104. | -1.9 | 9.588 | 60.7 | 58.3 |
| Angustus Labyrinthus: ESP_092853_0985 ESP_093183_0985 (Interval in Earth days: 26) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -81.4 | 296. | 16.7 | -2.01 | 60.3 | 63.9 |
| South Polar Residual Cap: ESP_093091_0910 ESP_093142_0910 (Interval in Earth days: 3) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -88.8 | 346. | 20.2 | 25.66 | 67.9 | 67.5 |
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