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.
| Sediment Fan in Crater: ESP_078808_1950 ESP_078663_1950 (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 | 14.65 | 338. | 5.39 | -8.68 | 46.3 | 46.7 |
| Nier Crater Central Depression: ESP_078724_2230 ESP_078856_2230 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 42.81 | 106. | 18.7 | -11.5 | 41.9 | 44.6 |
| Vent and Channel Northeast of Arsia Mons: ESP_078693_1730 ESP_079326_1730 (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 | -6.91 | 241. | 4.30 | -16.1 | 56.1 | 60.8 |
| Crater with Interior Slump in Arabia Terra: ESP_078807_2020 ESP_079229_2020 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.69 | 5.11 | 5.36 | -5.89 | 44.2 | 46.4 |
| Terra Cimmeria Dune Monitoring : ESP_078934_1655 ESP_078868_1655 (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 | -14.4 | 142. | 2.23 | 24.21 | 62.5 | 60.7 |
| Low Mound East of Echus Chasma: ESP_078784_1815 ESP_078929_1815 (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 | 1.567 | 276. | -8.4 | 7.57 | 52.9 | 52.6 |
| Lobate Apron in Phlegra Montes: ESP_078801_2165 ESP_078010_2165 (Interval in Earth days: 62) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.05 | 164. | 27.3 | -0.26 | 40.4 | 43.4 |
| Alluvial Fans and Grooved Terrain in Kasei Valles: ESP_078994_2040 ESP_078704_2040 (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 | 23.82 | 298. | 17.8 | -8.88 | 43.1 | 44.5 |
| Dune Monitoring in Northern Mid-Latitude Crater: ESP_078674_2295 ESP_078595_2295 (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 | 49.27 | 30.2 | 16.0 | -5.49 | 43.8 | 45.8 |
| Large Phyllosilicate Deposit near Magelhaens Crater: ESP_078827_1485 ESP_080449_1485 (Interval in Earth days: 126) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -30.9 | 185. | 2.50 | 18.61 | 73.0 | 73.9 |
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