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.
Unnamed Crater on Rim of Valles Marineris: ESP_017556_1650 ESP_018268_1650 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.7 | 297. | -12. | 0.635 | 63.2 | 63.2 |
Overlapping Lanslide Deposits Within Coprates Chasma: ESP_017688_1685 ESP_018321_1685 (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 | -11.5 | 292. | 3.48 | -20.3 | 60.5 | 62.6 |
Well-Preserved Impact Crater in Tempe Terra: ESP_017345_2200 ESP_017846_2200 (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 | 39.72 | 291. | -6.3 | 7.647 | 41.8 | 41.2 |
Volcanic Rootless Constructs in the Western Tartarus Colles: ESP_017389_2070 ESP_017890_2070 (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 | 26.51 | 171. | -9.2 | 7.114 | 42.8 | 42.5 |
Wrinkle Ridge in Hesperia Planum: ESP_017378_1530 ESP_018934_1530 (Interval in Earth days: 121) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -26.7 | 118. | 0 | -18.0 | 70.1 | 70.1 |
Polar Crater with Summer Ice: ESP_017510_2465 ESP_017945_2465 (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 | 66.39 | 99.7 | -0.4 | 14.50 | 49.4 | 48.4 |
Layered Terrain in Aeolis and Zephyria Regions: ESP_017680_1775 ESP_018102_1775 (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 | -2.31 | 149. | 4.54 | -12.8 | 54.6 | 56.5 |
Small Crater in Amazonis Planitia: ESP_017361_1830 ESP_018073_1830 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.024 | 219. | -6.7 | 4.499 | 51.3 | 52.3 |
Central Peak of an Impact Crater: ESP_017430_1910 ESP_018709_1910 (Interval in Earth days: 100) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 10.63 | 134. | -8.9 | 4.868 | 48.0 | 49.4 |
Channels and Streamlined Landforms: ESP_017666_1935 ESP_017732_1935 (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 | 13.13 | 169. | 9.37 | -13.0 | 46.2 | 48.1 |
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