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 with Iron Magnesium Phyllosilicate on Crater Floor: PSP_010419_2140 PSP_010841_2140 (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 | 33.71 | 17.1 | 16.6 | 1.275 | 49.7 | 55.7 |
Uplift in Oudemans Crater: ESP_011966_1700 ESP_012467_1700 (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 | -9.73 | 268. | 2.38 | 27.90 | 55.8 | 50.3 |
Possible MSL Rover Landing Site Eberswalde Crater: ESP_011265_1560 ESP_011331_1560 (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 | -23.8 | 326. | 20.4 | -1.11 | 60.2 | 61.4 |
Distributary Channel South of Ascraeus Mons: PSP_010872_1865 ESP_011373_1865 (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 | 6.197 | 254. | -2.2 | 20.12 | 55.7 | 55.8 |
Lonar Crater Ejecta: PSP_010800_2535 PSP_010787_2535 (Interval in Earth days: 1) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 73.30 | 39.0 | 20.1 | 6.293 | 68.3 | 68.9 |
Disrupted Terrain in Southeastern Cerberus Palus: ESP_011377_1835 ESP_011522_1835 (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 | 3.357 | 147. | -2.2 | 13.96 | 57.5 | 56.5 |
Valley Features and Light-Toned Deposits along Melas Region Southern Wall: ESP_011293_1710 ESP_019218_1710 (Interval in Earth days: 617) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.12 | 282. | 0.24 | -21.3 | 58.2 | 59.7 |
Well-Preserved Unnamed Crater in Acidalia Planitia: PSP_010579_2170 ESP_016104_2170 (Interval in Earth days: 431) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.66 | 329. | 4.65 | 19.26 | 52.8 | 40.8 |
Very Recent Small Crater: PSP_010772_2145 ESP_045136_2145 (Interval in Earth days: 2678) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 34.38 | 100. | 4.13 | -8.37 | 54.7 | 42.8 |
Phyllosilicate Ring in Terra Sirenum: PSP_010901_1510 ESP_055194_1510 (Interval in Earth days: 3452) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -28.9 | 187. | 0.35 | -23.2 | 66.4 | 62.6 |
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