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.
| High-Latitude Lobate Slope Features: ESP_062735_2495 ESP_062959_2495 (Interval in Earth days: 18) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 69.49 | 232. | -6.9 | 7.134 | 55.1 | 56.4 |
| Flow Deposits in Eastern Ladon Valles Basin: ESP_062745_1615 ESP_062956_1615 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -18.2 | 332. | 8.06 | -7.02 | 64.1 | 64.6 |
| Layered Material and Wall Spur in East Candor Chasma: ESP_062852_1725 ESP_069408_1725 (Interval in Earth days: 511) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.27 | 289. | 4.20 | -7.91 | 57.8 | 58.4 |
| Layers in Crater: ESP_062819_2570 ESP_062661_2570 (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 | 76.98 | 88.7 | 7.47 | -6.37 | 59.0 | 58.5 |
| Ridges in Tempe Terra: ESP_062905_2245 ESP_063538_2245 (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 | 43.94 | 275. | 3.89 | -22.0 | 46.9 | 56.7 |
| Dunes Dubbed Hazar South: ESP_062970_2550 ESP_062838_2550 (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 | 74.99 | 293. | -6.2 | 5.004 | 60.4 | 58.2 |
| Irregular Circular Depressions near Makhambet Crater: ESP_062798_2105 ESP_062864_2105 (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 | 30.04 | 320. | -6.4 | -25.4 | 46.1 | 48.4 |
| Sinuous Inverted Channel in Large Basin in East Arabia Terra: ESP_062808_2085 ESP_062874_2085 (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 | 28.26 | 45.7 | 8.60 | -12.7 | 45.0 | 47.3 |
| Chasma Boreale Megadunes: ESP_062652_2630 ESP_062547_2630 (Interval in Earth days: 8) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 82.75 | 315. | 7.01 | -8.83 | 61.2 | 61.3 |
| Dunes with Furrows: ESP_062912_2575 ESP_053918_2575 (Interval in Earth days: 701) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 77.16 | 75.5 | -7.2 | 7.214 | 61.0 | 58.0 |
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