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.
| Northern Sinus Meridiani Landforms : ESP_044731_1860 ESP_046287_1860 (Interval in Earth days: 122) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 5.896 | 358. | -4.8 | 11.63 | 48.7 | 49.2 |
| Lyot Crater Ejecta : ESP_044743_2290 ESP_044888_2290 (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 | 48.48 | 26.1 | -7.7 | 6.254 | 43.1 | 42.6 |
| High Thermal Inertia Depression in Ravi Vallis : ESP_044838_1790 ESP_045115_1790 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.66 | 317. | 7.72 | -6.36 | 51.2 | 51.7 |
| Streamlined Form in Lethe Vallis : ESP_044989_1845 ESP_045833_1845 (Interval in Earth days: 65) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.261 | 155. | 6.74 | -2.85 | 48.5 | 49.3 |
| Transverse Aeolian Ridges in Scandia Cavi : ESP_044722_2570 ESP_044405_2570 (Interval in Earth days: 25) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 76.93 | 226. | 2.31 | 28.96 | 55.5 | 52.8 |
| 360-Meter Crater on North Polar Layered Deposits : ESP_044845_2630 ESP_044674_2630 (Interval in Earth days: 13) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 82.98 | 94.7 | 5.72 | -8.84 | 60.1 | 59.9 |
| Troughs within East Candor Chasma : ESP_044773_1735 ESP_045406_1735 (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 | -6.63 | 292. | 13.5 | 29.45 | 54.4 | 51.4 |
| Topography and Geomorphology of Surface and Contacts in Astapus Colles : ESP_044754_2135 ESP_051980_2135 (Interval in Earth days: 563) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 33.14 | 86.8 | 2.02 | -17.1 | 40.4 | 39.7 |
| Polar Dunes : ESP_044760_2560 ESP_044918_2560 (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 | 76.09 | 271. | -0.1 | 16.86 | 55.3 | 55.2 |
| Possible Phyllosilicate Detection in a Small Crater Near Gale Crater Rim : ESP_044660_1740 ESP_045504_1740 (Interval in Earth days: 66) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.07 | 136. | 12.5 | 28.31 | 54.3 | 50.9 |
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