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.
Crater in North Elysium Planitia As Seen in THEMIS Image V21264008: PSP_008807_2145 PSP_009796_2145 (Interval in Earth days: 77) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 34.21 | 109. | 0.42 | -21.2 | 42.3 | 48.1 |
Isolated Gully at Intersection of Wrinkle Ridge and Crater Wall: PSP_008608_1510 PSP_009043_1510 (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 | -28.8 | 152. | -8.0 | 7.793 | 72.7 | 73.1 |
Olivine-Rich Deposits Off of the Ladon Impact Basin: PSP_009234_1675 PSP_009656_1675 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.5 | 336. | -0.6 | -16.3 | 62.8 | 63.8 |
Deposits Layered at Several Scales: PSP_009038_1745 PSP_010027_1745 (Interval in Earth days: 77) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.54 | 286. | 2.43 | -12.1 | 58.0 | 59.4 |
High-Latitude Exposure of North Polar Layered Deposits: PSP_009248_2675 PSP_009289_2675 (Interval in Earth days: 3) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 87.42 | 234. | -2.2 | -14.0 | 62.7 | 62.8 |
Curving Channel Near Rahway Valles: PSP_008607_1900 PSP_009042_1900 (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 | 10.11 | 175. | -8.0 | 8.124 | 48.9 | 49.1 |
Landslides in Ganges Chasma: PSP_009037_1715 PSP_009538_1715 (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 | -8.54 | 315. | -14. | 7.943 | 60.9 | 59.8 |
Seasonal Frost on Dunes: PSP_008847_2580 PSP_009256_2580 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 77.98 | 84.0 | -2.5 | -17.7 | 55.7 | 57.3 |
Eroded Mesa in Western Cydonia Region: PSP_008574_2210 PSP_009497_2210 (Interval in Earth days: 72) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.74 | 351. | 4.32 | -13.5 | 41.6 | 45.8 |
Athabasca Valles: PSP_009280_1905 PSP_009557_1905 (Interval in Earth days: 22) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 10.29 | 156. | 11.7 | -18.0 | 49.3 | 52.2 |
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