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 Peak with Summit Pit Inside 20-Kilometer Diameter Crater: PSP_006961_2195 PSP_007884_2195 (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 | 39.02 | 116. | 3.71 | -22.2 | 44.8 | 43.9 |
Exposure of High-Latitude Polar Layered Deposits Not Well-Observed: PSP_005139_0920 PSP_005269_0920 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.7 | 280. | 5.03 | 18.59 | 70.9 | 70.7 |
Deeply-Incised Channels in Mantled Crater Walls: PSP_006544_1460 PSP_010750_1460 (Interval in Earth days: 328) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -33.6 | 351. | 0 | -16.0 | 50.6 | 71.0 |
Complex Banded Terrain of Floor of Hellas Basin: PSP_006278_1410 PSP_010563_1410 (Interval in Earth days: 334) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.7 | 55.4 | 0 | 13.47 | 49.7 | 73.5 |
Exposure of Polar Layered Deposits Not Well Observed: PSP_005983_0920 ESP_023321_0920 (Interval in Earth days: 1351) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.9 | 278. | 8.62 | 15.55 | 83.6 | 77.5 |
Look For Unconformity at Base of Interior Layered Deposits: PSP_006519_1730 PSP_007020_1730 (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 | -6.74 | 311. | 0 | 9.783 | 37.5 | 42.3 |
Fresh Unnamed Crater with Ponded Materials and Gullies: PSP_005985_1455 ESP_013817_1455 (Interval in Earth days: 611) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -34.0 | 134. | 1.73 | 24.54 | 42.1 | 33.9 |
Juventae Chasma Layered Kieserite Deposit: PSP_006915_1760 PSP_007060_1760 (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 | -3.96 | 298. | 2.79 | 14.99 | 40.6 | 41.3 |
Syrtis Major Hydrated Crater Floor and Megabreccia in Central Pit: PSP_005842_1970 ESP_011538_1970 (Interval in Earth days: 444) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.03 | 71.8 | 6.01 | -18.2 | 41.4 | 61.2 |
Gullies: PSP_006821_1270 ESP_024121_1270 (Interval in Earth days: 1349) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -52.6 | 351. | -0.1 | -25.5 | 68.9 | 63.9 |
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