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.
| Light-Toned Possible Fans at Base of Crater Wall: ESP_031127_1500 ESP_075647_1500 (Interval in Earth days: 3469) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -29.6 | 236. | 2.27 | -8.59 | 35.1 | 36.3 |
| Possible Fluvial Features in Golden Crater: ESP_031005_1575 ESP_039405_1575 (Interval in Earth days: 654) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -22.0 | 326. | -5.8 | 8.33 | 37.4 | 43.5 |
| Reull Vallis and Tongue-Shaped Landform in the Centauri Montes: ESP_031119_1405 ESP_031264_1405 (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 | -39.0 | 97.1 | -11. | 2.562 | 37.6 | 35.9 |
| Flows Associated with Mojave Crater Secondaries: ESP_031229_1895 ESP_040196_1895 (Interval in Earth days: 699) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.550 | 326. | 1.62 | 22.38 | 48.5 | 46.8 |
| Possible Preserved Impact Melt Flow on the Ejecta of Bakhuysen Crater: ESP_031201_1555 ESP_031056_1555 (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 | -24.3 | 13.8 | 17.1 | 1.41 | 33.5 | 36.1 |
| Northern Hellas Planitia Layered Bedrock: ESP_031120_1505 ESP_031898_1505 (Interval in Earth days: 61) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -28.9 | 67.3 | 0 | -13.4 | 35.4 | 34.8 |
| Impact Crater with Central Peak: ESP_031226_1820 ESP_067015_1820 (Interval in Earth days: 2789) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.009 | 50.0 | -5.7 | 8.953 | 44.3 | 42.4 |
| South Polar Layered Deposit Spiral Troughs during Katabatic Wind Season: ESP_031048_0945 ESP_031100_0945 (Interval in Earth days: 4) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -85.4 | 289. | -13. | 2.826 | 65.5 | 64.1 |
| Light-Toned Stratified Materials in Melas Chasma: ESP_031125_1670 ESP_031903_1670 (Interval in Earth days: 61) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.0 | 289. | -4.6 | -18.9 | 38.4 | 33.6 |
| USGS Dune Database Entry Number 2226-767: ESP_031260_1030 ESP_031062_1030 (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 | -76.6 | 223. | -13. | 3.747 | 58.8 | 57.0 |
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