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.
| Reull Vallis: ESP_067317_1405 ESP_067726_1405 (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 | -39.4 | 96.4 | -6.7 | 3.611 | 44.5 | 49.4 |
| Fractures in Chryse Planitia: ESP_067348_1980 ESP_067546_1980 (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 | 17.85 | 321. | 7.95 | -17.0 | 47.8 | 47.9 |
| Well-Preserved Impact Crater: ESP_067346_2140 ESP_076380_2140 (Interval in Earth days: 703) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 33.58 | 15.6 | -6.3 | 2.816 | 58.7 | 53.7 |
| Phlegra Montes: ESP_067367_2165 ESP_067710_2165 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.33 | 162. | -7.7 | 8.518 | 60.4 | 55.4 |
| Idaeus Fossae: ESP_067388_2165 ESP_067599_2165 (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 | 36.02 | 309. | -4.8 | 22.66 | 59.8 | 55.5 |
| Gullies on Mound in Nereidum Montes: ESP_067467_1350 ESP_067876_1350 (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 | -44.5 | 324. | -4.3 | 8.455 | 48.9 | 54.5 |
| Oyama Crater Rim: ESP_067664_2045 ESP_067796_2045 (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 | 24.09 | 339. | 7.76 | -5.86 | 48.5 | 48.5 |
| Layering in Argyre Planitia: ESP_067573_1245 ESP_066966_1245 (Interval in Earth days: 47) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -55.2 | 314. | -0.7 | 15.46 | 56.9 | 47.7 |
| Valleys in Tyrrhena Terra: ESP_067594_1635 ESP_073951_1635 (Interval in Earth days: 495) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -16.2 | 95.0 | -2.2 | 18.88 | 39.7 | 52.0 |
| Channel in Wall of Orson Welles Crater: ESP_067322_1790 ESP_075301_1790 (Interval in Earth days: 621) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.88 | 314. | -7.4 | 16.47 | 40.7 | 43.7 |
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