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.
| Layers in Spallanzani Crater: ESP_013041_1215 ESP_013120_1215 (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 | -58.1 | 86.8 | 5.04 | 26.10 | 48.1 | 45.8 |
| Well-Preserved 3 Kilometer Diameter Impact Crater: ESP_012991_1335 ESP_013624_1335 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -45.9 | 9.53 | 3.76 | -12.3 | 44.3 | 40.8 |
| Pit with Layered Walls in Mid-Latitude Mantling Unit: ESP_013951_1225 ESP_021731_1225 (Interval in Earth days: 606) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -57.3 | 82.3 | 2.27 | -20.0 | 47.0 | 49.7 |
| Layering in Crater: ESP_013057_1825 ESP_013769_1825 (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 | 2.613 | 1.41 | 3.63 | 16.95 | 51.9 | 42.7 |
| North Wall of Ritchey Crater: ESP_013125_1520 ESP_013758_1520 (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 | -27.9 | 309. | 0.17 | -22.9 | 41.2 | 37.0 |
| Ridges at the Edge of the Layered Deposits within Reynolds Crater: ESP_013169_1055 ESP_013301_1055 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -74.2 | 200. | -3.6 | -17.2 | 56.4 | 57.0 |
| Diverse Layers and Morphologies in North Rim of Hellas Planitia: ESP_013490_1525 ESP_058166_1530 (Interval in Earth days: 3481) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.3 | 64.2 | -5.3 | 5.215 | 37.6 | 30.5 |
| Sublimation Scallops: ESP_013873_1225 ESP_014005_1225 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -57.0 | 51.1 | 6.96 | -20.3 | 45.9 | 48.6 |
| Possible Fan Delta: ESP_013531_2140 ESP_022036_2140 (Interval in Earth days: 663) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 33.87 | 17.5 | -8.5 | 21.35 | 68.7 | 68.8 |
| Edge of Fluidized Ejecta Rampart with Great Phyllosilicate Signature: ESP_012909_1680 ESP_013331_1680 (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 | -11.9 | 83.6 | 3.17 | -12.0 | 47.1 | 43.1 |
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