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.
| Candidate ExoMars Landing Site in Oxia Planum: ESP_088078_2000 ESP_088012_2000 (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 | 19.56 | 334. | -28. | -7.03 | 48.3 | 46.2 |
| Dune Monitoring in Northern Mid-Latitude Crater: ESP_088171_2295 ESP_088395_2295 (Interval in Earth days: 18) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 49.11 | 309. | -5.5 | 19.83 | 44.5 | 42.6 |
| Pedestal Crater Marginal Pits: ESP_088126_2400 ESP_088205_2400 (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 | 59.79 | 96.3 | -9.1 | 6.586 | 47.8 | 46.5 |
| Planned ExoMars Landing Site in Oxia Planum: ESP_088157_1975 ESP_088447_1975 (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 | 17.33 | 336. | -8.6 | 8.83 | 47.5 | 46.8 |
| Crater Infill: ESP_088354_1870 ESP_088565_1870 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 6.953 | 356. | 10.0 | -5.16 | 51.1 | 52.6 |
| North-Pole-Facing Deposit in Crater Associated with Headwall Erosion: ESP_088226_2150 ESP_088661_2150 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 34.60 | 249. | -5.8 | 17.63 | 43.6 | 42.7 |
| Group of Channels along Old Crater Wall: ESP_088288_2130 ESP_088499_2130 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 32.59 | 357. | -6.7 | -18.5 | 44.0 | 45.7 |
| Patterned Ground in Elysium Planitia: ESP_088335_1845 ESP_088546_1845 (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 | 4.634 | 156. | 3.81 | -11.4 | 52.6 | 54.2 |
| Distinct Crater Wall Layers in Oxia Planum: ESP_088236_1995 ESP_087946_1995 (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 | 19.08 | 338. | -1.7 | -16.6 | 46.5 | 47.0 |
| Dune Monitoring in Northern Mid-Latitude Crater: ESP_088230_2400 ESP_088454_2400 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 59.81 | 135. | -4.2 | 14.96 | 47.5 | 46.2 |
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