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.
Layered Deposits in Crater in Western Arabia Terra: ESP_017936_1890 ESP_060489_1890 (Interval in Earth days: 3315) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.810 | -0.9 | 0.22 | -9.82 | 49.5 | 41.2 |
Amazonis Planitia: ESP_017836_1970 ESP_017981_1970 (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 | 16.64 | 209. | -11. | 2.253 | 46.8 | 46.0 |
Clay Diversity on Flank of Mawrth Vallis: ESP_017897_2045 ESP_018530_2045 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.08 | 341. | 4.44 | -14.5 | 43.4 | 46.8 |
Impact Crater Teetering on the Edge of a Canyon: ESP_017740_1680 ESP_025810_1680 (Interval in Earth days: 629) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.7 | 312. | 5.84 | -8.97 | 60.6 | 56.8 |
Northern Hemisphere Gullies on a West-Facing Crater Slope: ESP_017405_2270 ESP_017827_2270 (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 | 46.67 | 90.1 | 7.09 | -4.59 | 41.7 | 43.0 |
Bacolor Crater Gullies: ESP_017681_2135 ESP_017971_2135 (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 | 32.97 | 118. | -8.0 | 14.61 | 42.4 | 41.1 |
Pit Craters in North Polar Layered Deposit: ESP_017376_2645 ESP_018918_2645 (Interval in Earth days: 120) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 84.39 | 134. | 0.70 | 16.29 | 60.4 | 65.5 |
Sinuous Ridge Witin the Upper Reach of Maadim Vallis: ESP_017600_1540 ESP_017745_1540 (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 | -25.9 | 176. | 0 | 13.55 | 70.4 | 70.0 |
Slope Streaks in Lycus Sulci: ESP_017585_2080 ESP_025734_2080 (Interval in Earth days: 635) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 27.95 | 220. | -8.6 | 8.376 | 42.9 | 38.9 |
Alba Region Valleys: ESP_017676_2260 ESP_017742_2260 (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 | 45.51 | 251. | 7.35 | -8.07 | 41.6 | 42.9 |
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