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.
| Spider Terrain: ESP_041065_0970 ESP_041039_0970 (Interval in Earth days: 2) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -82.7 | 26.7 | 8.49 | -7.53 | 74.9 | 75.5 |
| Crater with Steep Gullied Slopes: ESP_041021_1460 ESP_041878_1460 (Interval in Earth days: 67) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -33.7 | 130. | 1.04 | 20.98 | 39.5 | 50.7 |
| Circular Ridges and Troughs: ESP_040794_2185 ESP_041071_2185 (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 | 38.33 | 199. | -5.7 | -25.3 | 61.2 | 58.5 |
| Morphometry of Secondary Impact Craters: ESP_040927_1880 ESP_041428_1880 (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 | 7.739 | 171. | 0.52 | 25.96 | 38.9 | 34.2 |
| Icy Scarp: ESP_040772_1215 ESP_041062_1215 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -58.0 | 93.6 | -4.8 | 13.05 | 51.8 | 55.0 |
| Layering on Floor of Orson Welles Crater: ESP_040790_1805 ESP_056996_1805 (Interval in Earth days: 1263) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.309 | 314. | -20. | 5.758 | 38.3 | 48.2 |
| Surface Features Emanating from Alcove in Deuteronilus Mensae: ESP_040787_2210 ESP_041222_2210 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.73 | 30.1 | -6.7 | 26.93 | 63.2 | 55.1 |
| Terracing Inside and Outside Degraded Crater Rim: ESP_040785_2135 ESP_041286_2135 (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 | 33.38 | 84.9 | 0.81 | 23.90 | 57.1 | 49.1 |
| Spider Terrain: ESP_040789_0950 ESP_049334_0950 (Interval in Earth days: 666) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -85.0 | 13.6 | 3.96 | -6.39 | 72.8 | 69.5 |
| Patterned Ground on Braided Channel Near Steep Scarp: ESP_041036_1460 ESP_040601_1460 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -33.7 | 80.7 | 3.24 | -29.2 | 39.5 | 38.6 |
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