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 Features in Deuteronilus Mensae: ESP_016313_2265 ESP_016590_2265 (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 | 46.17 | 23.3 | 8.14 | -8.96 | 44.5 | 44.6 |
| Degradation of Old Crater Rim on Northwest Slope of Acheron Fossae: ESP_016873_2185 ESP_017018_2185 (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 | 38.30 | 218. | -8.3 | 1.584 | 42.0 | 41.0 |
| Wallrock Spurs That Are Alligned and Extend Into Melas Chasma: ESP_016528_1705 ESP_016884_1705 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.28 | 282. | -8.6 | 5.446 | 52.4 | 54.7 |
| Field of Small Volcanoes Northeast of Ascraeus Mons: ESP_016489_1945 ESP_017122_1945 (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 | 14.35 | 263. | 7.23 | -11.9 | 41.0 | 45.5 |
| Ridged Material in Viking Image 693A34: ESP_016359_1910 ESP_016992_1910 (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 | 10.86 | 212. | 13.8 | -2.12 | 40.6 | 45.5 |
| Light-Toned Layering in Noctis Labyrinthus Pit: ESP_016898_1695 ESP_019377_1695 (Interval in Earth days: 193) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -10.4 | 261. | -4.2 | -21.4 | 56.2 | 59.9 |
| Cerberus Fossae Region Seen in THEMIS Image: ESP_016651_1895 ESP_044026_1895 (Interval in Earth days: 2134) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.408 | 161. | 2.65 | 18.14 | 43.8 | 44.8 |
| Juventae Chasma Mound: ESP_016567_1755 ESP_017279_1755 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.69 | 296. | 0 | 16.66 | 49.7 | 53.7 |
| Debris Apron Source Area: ESP_016673_2255 ESP_017741_2255 (Interval in Earth days: 83) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 45.29 | 276. | -1.2 | 10.92 | 43.4 | 41.3 |
| Mesa Island in East Acidalia Planitia: ESP_016301_2250 ESP_016578_2250 (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 | 44.70 | 352. | -3.9 | -20.7 | 44.9 | 45.2 |
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