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 Uplift of a Large Crater North of Hellas Planitia: ESP_014439_1505 ESP_020742_1505 (Interval in Earth days: 491) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -29.2 | 74.5 | 5.54 | 18.53 | 36.0 | 53.2 |
Ridges in Candor Chasma: ESP_014286_1735 ESP_020299_1735 (Interval in Earth days: 469) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.39 | 288. | 1.34 | -12.9 | 34.8 | 56.1 |
Small Crater on Lobate Apron: ESP_014398_1305 ESP_020490_1305 (Interval in Earth days: 475) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -49.4 | 118. | -7.6 | 7.572 | 47.0 | 64.0 |
Central Peak Surrounded by Fan: ESP_014320_1465 ESP_022113_1465 (Interval in Earth days: 607) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -33.0 | 84.3 | 0 | 20.54 | 36.9 | 35.6 |
Cones in Acidalia Region: ESP_014258_2210 ESP_022974_2210 (Interval in Earth days: 679) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.53 | 326. | 6.91 | 26.01 | 63.5 | 63.2 |
Ophir Chasma Interior Deposits: ESP_014352_1760 ESP_021499_1760 (Interval in Earth days: 557) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.01 | 287. | -4.3 | -21.7 | 35.5 | 51.9 |
Western Edge of Layered Mound in Juventae Chasma: ESP_014378_1755 ESP_020470_1755 (Interval in Earth days: 475) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.47 | 297. | -4.8 | 16.67 | 35.3 | 53.4 |
Very Fresh 1-Kilometer Diameter Impact Crater: ESP_014405_1635 ESP_021776_1635 (Interval in Earth days: 575) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -16.2 | 281. | -5.4 | 26.42 | 33.9 | 41.2 |
Well-Preserved 7-Kilometer Diameter Gullied Crater in Newton Region: ESP_014395_1425 ESP_022188_1425 (Interval in Earth days: 607) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.2 | 198. | -8.2 | 9.964 | 39.9 | 36.2 |
Fans and Polygons: ESP_014266_0925 ESP_014410_0925 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.3 | 167. | 8.77 | 22.08 | 73.6 | 74.6 |
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