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.
| Layered Material within Small Crater in Nilosyrtis Mensae: ESP_017907_2125 ESP_053787_2125 (Interval in Earth days: 2796) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 32.07 | 68.2 | -5.4 | 6.933 | 42.7 | 41.6 |
| Fresh Looking Crater West of Erebus Montes in Arcadia Planitia: ESP_017784_2185 ESP_018272_2185 (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 | 38.05 | 184. | 7.20 | -20.5 | 41.1 | 45.1 |
| Rampart Crater Sample: ESP_018010_2455 ESP_018656_2455 (Interval in Earth days: 51) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 65.42 | 128. | 2.96 | 17.4 | 49.0 | 51.6 |
| Central Peak of a Large Crater in Acidalia Planitia: ESP_017700_2160 ESP_018412_2160 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.81 | 319. | -4.0 | 7.082 | 42.0 | 43.2 |
| Ridges and Flow-Like Forms: ESP_017734_2075 ESP_071880_2075 (Interval in Earth days: 4219) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 27.32 | 111. | -1.2 | 16.1 | 42.7 | 47.9 |
| Fault Scarp South of Arsia Mons: ESP_017769_1685 ESP_017914_1685 (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 | -11.6 | 241. | -9.1 | 6.675 | 61.5 | 60.8 |
| Valleys and Layering along Melas Region: ESP_018018_1705 ESP_026866_1705 (Interval in Earth days: 689) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.55 | 283. | -6.8 | -17.8 | 60.4 | 60.2 |
| Well-Preserved Impact Crater with Ridges: ESP_017975_1705 ESP_025557_1705 (Interval in Earth days: 590) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.51 | 16.4 | 0.77 | 18.29 | 59.9 | 51.6 |
| Shallow Channel Cutting through a Crater in CTX Image: ESP_017740_2230 ESP_024900_2230 (Interval in Earth days: 558) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 42.79 | 305. | 3.34 | 18.77 | 41.7 | 42.4 |
| Volcanic Rootless Constructs in the Western Tartarus Colles: ESP_017956_2065 ESP_018668_2065 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 26.37 | 171. | -9.0 | 6.491 | 44.1 | 45.2 |
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