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.
| Well-Preserved Crater North of Hellas Planitia : ESP_052218_1635 ESP_060183_1635 (Interval in Earth days: 620) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -16.1 | 74.3 | -6.3 | 5.878 | 58.1 | 48.6 |
| A Window into the Past: ESP_051841_1750 ESP_051986_1750 (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 | -5.16 | 283. | 10.4 | 27.06 | 46.8 | 46.9 |
| Outlet Breach in Small Crater: ESP_051967_1800 ESP_052112_1800 (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 | 0.102 | 84.6 | -5.4 | 13.68 | 46.1 | 46.0 |
| Cracked Channel-Filling Deposit or Slumped Ejecta: ESP_051969_2095 ESP_052114_2095 (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 | 29.20 | 25.8 | 1.30 | 16.21 | 37.9 | 36.8 |
| Sinuous Ridges and Valleys in Peridier Crater: ESP_051901_2055 ESP_052046_2055 (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 | 25.27 | 83.6 | -8.9 | 6.983 | 38.6 | 37.6 |
| Arabia Terra Dune Ripple Monitoring: ESP_051890_1815 ESP_052167_1815 (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 | 1.367 | 26.2 | 0.06 | -23.9 | 44.5 | 48.4 |
| Crater-Cored Island in Lava Flow Field: ESP_051882_2040 ESP_052383_2040 (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 | 23.81 | 241. | 7.04 | 25.48 | 37.3 | 37.1 |
| Down-Cutting Channel with Possible Inverted Channel: ESP_051995_1525 ESP_052140_1525 (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 | -27.4 | 43.8 | -6.3 | 11.55 | 64.0 | 64.4 |
| Anomalous Terrain on Olympus Mons Aureole : ESP_051896_1975 ESP_051751_1975 (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 | 17.22 | 217. | 26.1 | 11.42 | 36.5 | 37.2 |
| Mounds West of Schiaparelli Crater: ESP_051983_1745 ESP_052128_1745 (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 | -5.43 | 9.43 | -16. | 2.566 | 50.1 | 50.0 |
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