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.
| Canyon Walls in Coprates Chasma: ESP_088646_1655 ESP_088857_1655 (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 | -14.1 | 306. | 4.01 | -9.22 | 64.2 | 64.9 |
| A Fissure and Channel near Pavonis Mons: ESP_086934_1775 ESP_087435_1775 (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 | -2.54 | 247. | -7.1 | 24.56 | 49.0 | 51.0 |
| Ring-Shaped Mounds in Ceraunius : ESP_086815_2115 ESP_087092_2115 (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 | 31.79 | 249. | 16.7 | -7.37 | 40.6 | 42.5 |
| 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 |
| Dune Survey: ESP_088162_2540 ESP_088676_2540 (Interval in Earth days: 41) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 73.92 | 186. | -0.7 | 14.11 | 53.6 | 53.3 |
| Dune Monitoring in North Mid-Latitude Crater: ESP_088261_2420 ESP_088182_2420 (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 | 61.94 | 6.66 | 6.67 | -7.68 | 47.4 | 48.6 |
| 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 |
| Dune Field: ESP_088070_2535 ESP_088413_2535 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 73.41 | 178. | 0.65 | -15.8 | 53.4 | 54.6 |
| Dune Survey: ESP_088329_2415 ESP_088817_2415 (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 | 61.26 | 311. | -0.1 | -21.9 | 47.8 | 51.3 |
| 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 |
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