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.
| Crossing Wrinkle Ridges and Secondaries in Hesperia Planum: ESP_016310_1545 ESP_016666_1545 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -25.2 | 115. | 3.44 | 15.21 | 59.1 | 62.7 |
| Lobate Tongue Terminus in CTX Image: ESP_016418_2255 ESP_017130_2255 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 45.06 | 38.1 | -2.1 | 10.57 | 44.3 | 41.3 |
| Crater West of Niesten Crater: ESP_016510_1515 ESP_019279_1515 (Interval in Earth days: 216) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -28.2 | 56.2 | -2.9 | 14.98 | 64.0 | 66.9 |
| Small Volcano in Tharsis Region: ESP_016806_2005 ESP_016872_2005 (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 | 20.15 | 247. | 16.4 | -3.58 | 40.3 | 42.2 |
| Gordii Dorsum: ESP_016847_1910 ESP_017559_1910 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 10.61 | 211. | -2.9 | 6.107 | 44.9 | 47.3 |
| Relatively Fresh Crater Cut by Erosion: ESP_016738_1730 ESP_019296_1730 (Interval in Earth days: 200) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.05 | 309. | -7.3 | 16.52 | 53.0 | 55.8 |
| Interesting Crater Ejecta in Columbus Crater: ESP_016861_1505 ESP_017639_1505 (Interval in Earth days: 60) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -29.3 | 193. | 1.16 | -12.7 | 68.3 | 73.7 |
| Isolated Layered Mound in Trough Between Layered Benches in Terby Crater: ESP_016628_1520 ESP_016773_1520 (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 | -27.6 | 74.4 | 0.18 | 16.62 | 64.9 | 65.4 |
| Columnar Jointing in West Wall of Crater in Marte Vallis: ESP_016360_2020 ESP_016505_2020 (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 | 21.55 | 184. | 7.23 | 21.49 | 39.4 | 38.5 |
| Possible MSL Rover Landing Site in Northeast Syrtis Region: ESP_016575_1980 ESP_016509_1980 (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 | 17.81 | 77.2 | -17. | 2.958 | 42.7 | 40.7 |
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