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 Landing Site for 2020 Mission in Hypanis Valles Delta: ESP_041436_1920 ESP_041858_1920 (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 | 12.02 | 314. | -0.1 | -24.4 | 37.7 | 39.3 |
| Possible Future Landing Site North of Echus Chaos: ESP_041358_1955 ESP_041213_1955 (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 | 15.17 | 284. | -3.7 | -19.6 | 39.6 | 41.7 |
| Possible Degraded Crater on South Polar Layered Deposits: ESP_041218_0925 ESP_041309_0925 (Interval in Earth days: 7) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.6 | 243. | 3.20 | 9.973 | 83.4 | 83.5 |
| Possible Crater in South Polar Layered Deposits: ESP_041150_0920 ESP_041046_0920 (Interval in Earth days: 8) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.7 | 240. | 20.0 | 6.466 | 80.0 | 79.8 |
| Protonilus Region Terraces: ESP_041129_2210 ESP_041406_2210 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.73 | 51.7 | 5.59 | -14.1 | 57.6 | 55.0 |
| Layered Crater Wall in Northwest Hellas Planitia: ESP_041116_1470 ESP_041393_1470 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -32.6 | 56.9 | -0.3 | -23.1 | 40.2 | 45.4 |
| Gullies on Western Slope of Crater on Edge of Ptolemaeus Crater: ESP_041256_1330 ESP_041335_1330 (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 | -46.5 | 200. | -29. | -2.33 | 52.4 | 51.8 |
| Dark Capped Sinuous Ridges Aligned Radially around Basin: ESP_041437_1365 ESP_041358_1365 (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 | -43.3 | 292. | 22.4 | -4.33 | 49.8 | 50.2 |
| Line of Mounds East of Chryse Planitia: ESP_041145_2125 ESP_042002_2125 (Interval in Earth days: 67) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 32.23 | 336. | 3.48 | 17.97 | 51.3 | 41.9 |
| USGS Dune Database Entry Number 0081-097 Changes: ESP_041289_1900 ESP_041355_1900 (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 | 9.714 | 8.19 | 8.12 | -15.2 | 36.9 | 38.4 |
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