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.
| Arabia Terra Crater Floor Dune Changes: ESP_022775_1930 ESP_022498_1930 (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 | 12.90 | 9.07 | -25. | 2.217 | 47.8 | 49.6 |
| The Crazy Floor of the Hellas Basin: ESP_023234_1460 ESP_024091_1460 (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 | -33.5 | 81.5 | 0.57 | 28.11 | 36.3 | 46.4 |
| Starburst Spiders at a South Polar Cracked and Gullied Site: ESP_023117_0980 ESP_022998_0980 (Interval in Earth days: 9) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -81.6 | 66.2 | -18. | -2.77 | 70.6 | 67.8 |
| Fan-Shaped Deposit in a Valles Marineris Trough: ESP_022949_1650 ESP_030518_1650 (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 | -14.9 | 299. | -1.6 | 21.10 | 32.0 | 42.9 |
| Possible Light-Toned Layered Unit along Noctis Region Depression: ESP_022647_1690 ESP_023069_1690 (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 | -10.6 | 263. | 7.19 | -12.3 | 34.6 | 33.0 |
| Active Dune Gully in Matara Crater: ESP_022471_1300 ESP_022616_1300 (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 | -49.4 | 34.7 | 0.78 | 14.28 | 40.1 | 39.4 |
| Reticulate Bedform Change Detection West of Arsia Mons: ESP_022648_1735 ESP_022503_1735 (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 | -6.30 | 235. | 19.6 | 0.712 | 35.4 | 38.3 |
| Gullies and Lobate Material in a Crater in Nereidum Montes: ESP_022540_1405 ESP_023173_1405 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.0 | 308. | 3.88 | -14.2 | 35.4 | 39.5 |
| Central Uplift of Impact Crater: ESP_022454_1470 ESP_022599_1470 (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 | -32.5 | 136. | -0.5 | 16.53 | 34.4 | 32.5 |
| Coprates Chasma Dune Changes: ESP_022369_1685 ESP_023002_1685 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.4 | 293. | 4.01 | -17.8 | 37.5 | 33.6 |
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