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.
| Polar Barchan Dune Changes : ESP_045855_2565 ESP_046053_2565 (Interval in Earth days: 15) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 76.52 | 253. | 8.97 | -5.39 | 66.4 | 70.4 |
| Western Half of Rayed Pebas Crater : ESP_045997_1775 ESP_046142_1775 (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 | -2.61 | -0.9 | -6.3 | 8.161 | 51.8 | 50.7 |
| Crater with Channel : ESP_046123_1790 ESP_055129_1790 (Interval in Earth days: 702) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.88 | 158. | -3.1 | -28.7 | 51.1 | 54.8 |
| Louth Crater Ice Mound : ESP_045887_2505 ESP_045439_2505 (Interval in Earth days: 35) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 70.22 | 103. | 18.0 | -8.26 | 62.4 | 58.1 |
| Small Tributary Deposit and Transverse Aeolian Ridges in Nirgal Vallis : ESP_045814_1520 ESP_046592_1520 (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 | -27.6 | 317. | 5.48 | -4.70 | 63.3 | 57.8 |
| Syria Planum Bedform and Albedo Changes : ESP_046080_1655 ESP_046502_1655 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.2 | 252. | 22.2 | 7.064 | 53.8 | 53.2 |
| Scarps in Utopia Planitia : ESP_045808_2090 ESP_046309_2090 (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 | 28.74 | 114. | 0 | 14.75 | 46.7 | 51.0 |
| Fan in Rahe Crater : ESP_045829_2050 ESP_062642_2050 (Interval in Earth days: 1310) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.90 | 262. | -7.1 | -28.4 | 47.2 | 47.8 |
| High-Latitude Exposure of North Polar Layered Deposits : ESP_046056_2725 ESP_045567_2725 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 87.67 | 21.5 | -18. | -29.2 | 81.3 | 75.2 |
| Fractures in Utopia Planitia : ESP_046151_2140 ESP_046573_2140 (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 | 33.84 | 108. | 4.82 | -6.29 | 51.2 | 57.7 |
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