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.
Central Peak of an Impact Crater in Promethei Terra: ESP_020846_1400 ESP_029536_1400 (Interval in Earth days: 677) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.5 | 118. | 1.54 | -24.2 | 55.4 | 59.0 |
Material Flowing Through Gap in Crater Rim East of Hellas Planitia: ESP_020543_1345 ESP_029246_1345 (Interval in Earth days: 678) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -45.2 | 111. | -0.3 | 25.69 | 62.1 | 61.5 |
Fresh 3-Kilometer Diameter Rayed Crater on Preexisting Crater Terrace: ESP_020752_1500 ESP_021596_1500 (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 | -29.5 | 163. | 0.50 | -27.6 | 54.5 | 45.8 |
Floor of East Candor Chasma: ESP_020668_1720 ESP_020813_1720 (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 | -7.93 | 293. | 6.15 | 22.34 | 53.6 | 51.7 |
Faults in Claritas Fossae: ESP_020775_1535 ESP_021487_1535 (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 | -26.1 | 254. | 4.50 | 17.44 | 53.5 | 43.8 |
Crater Floor with Depressions Containing Circular Mesas: ESP_020535_1510 ESP_038020_1510 (Interval in Earth days: 1363) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -28.5 | 328. | -15. | -3.02 | 58.0 | 60.2 |
Well-Preserved Large Impact Crater in Terra Sirenum: ESP_020777_1590 ESP_020843_1590 (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 | -20.9 | 199. | 5.03 | -16.6 | 52.9 | 53.9 |
Small Crater with Gullies and a Bright Fan: ESP_020897_1455 ESP_021609_1455 (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 | -34.2 | 165. | -3.8 | 6.575 | 53.8 | 43.0 |
Mesa in Acidalia Planitia: ESP_020587_2250 ESP_047105_2250 (Interval in Earth days: 2066) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 44.76 | 338. | 0.81 | 27.13 | 71.0 | 67.9 |
Debris Flow: ESP_020558_2215 ESP_020835_2215 (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 | 41.17 | 50.8 | -3.6 | -22.7 | 69.0 | 73.7 |
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