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.
Two Overlapping Icy Flows in a Canyon of Ismeniae Fossae: PSP_004142_2215 ESP_012396_2215 (Interval in Earth days: 643) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.90 | 42.0 | -7.8 | 7.037 | 77.3 | 76.1 |
Ring and Cone Structures and Platy-Ridged Terrain in Amazonis Planitia: PSP_003701_1915 PSP_004202_1915 (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 | 11.50 | 204. | 0.18 | 23.98 | 59.1 | 54.9 |
Huo Hsing Vallis: PSP_003495_2065 PSP_003561_2065 (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 | 26.43 | 66.5 | 5.45 | -14.4 | 66.3 | 67.9 |
Potential Currently-Active Gullies in Fresh Crater: PSP_003939_1420 ESP_012549_1420 (Interval in Earth days: 671) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.6 | 192. | 7.82 | 27.83 | 44.6 | 47.0 |
Intriguing Dark Dunes in Proctor Crater: PSP_003101_1320 ESP_011909_1320 (Interval in Earth days: 686) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -47.7 | 30.6 | 22.7 | -2.86 | 58.7 | 61.9 |
Light Toned Ridges in Meridiani Region: PSP_003682_1805 PSP_003972_1805 (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 | 0.329 | 5.15 | -0.2 | 29.79 | 54.2 | 50.0 |
Channel Flow: PSP_003978_1715 PSP_004334_1715 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.28 | 205. | -3.3 | 7.629 | 48.8 | 44.2 |
Circular Feature Which Looks Like Subsidence and Collapse: PSP_003728_0930 ESP_030073_0930 (Interval in Earth days: 2053) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -86.7 | 248. | 0.32 | 12.38 | 69.8 | 69.9 |
Light-Toned Deposit in Tithonium Chasma: PSP_003514_1755 PSP_005848_1755 (Interval in Earth days: 182) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.60 | 271. | 6.07 | -6.81 | 52.9 | 34.2 |
Gully Previously Identified in MOC Image M08-00012: PSP_003842_1245 PSP_005319_1245 (Interval in Earth days: 115) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -55.2 | 324. | 1.51 | -26.3 | 51.0 | 48.7 |
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