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.
Characterize Surface Hazards and Science of Possible MSL Rover Landing Site: PSP_008680_2050 PSP_009260_2050 (Interval in Earth days: 46) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.63 | 340. | -11. | 19.88 | 44.5 | 43.4 |
Textured Plain in Arcadia Planitia: PSP_008566_2285 ESP_016069_2285 (Interval in Earth days: 585) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 48.18 | 209. | -4.0 | -26.0 | 43.4 | 49.7 |
Central Peak of Bonestell Crater: PSP_008733_2225 ESP_018372_2225 (Interval in Earth days: 752) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 41.96 | 329. | -2.7 | 11.77 | 42.5 | 43.0 |
Dune Interaction with Topography in Ganges Chasma: PSP_008536_1725 PSP_009604_1725 (Interval in Earth days: 83) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.40 | 314. | 8.72 | -5.05 | 56.9 | 60.1 |
Merging Lobate Debris Aprons of Deuteronilus Mensae: PSP_008744_2240 PSP_009535_2240 (Interval in Earth days: 62) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 43.76 | 29.3 | -6.2 | 15.83 | 43.0 | 43.5 |
Polar Layered Deposits Unconformity: PSP_009203_2625 PSP_009585_2625 (Interval in Earth days: 30) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 82.34 | 79.7 | -7.1 | 7.321 | 58.9 | 59.8 |
Unnamed Faded Rayed Crater in Elysium Planitia: PSP_009123_2040 ESP_016560_2040 (Interval in Earth days: 579) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.94 | 122. | 3.65 | 21.08 | 44.6 | 38.5 |
Layered Deposits in Crater in Arabia Terra: PSP_008520_2085 PSP_009232_2085 (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 | 28.00 | 27.9 | 1.13 | -16.8 | 42.3 | 45.8 |
Very Fresh Small Crater in Arabia Region: PSP_009206_1920 ESP_062941_1915 (Interval in Earth days: 4187) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 11.71 | 17.8 | 3.16 | -6.38 | 49.2 | 50.5 |
Bedrock Exposed in Crater Wall in Acidalia Region: PSP_009036_2250 ESP_062850_2250 (Interval in Earth days: 4193) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 44.59 | 335. | -3.5 | 15.73 | 43.4 | 45.5 |
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