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.
Avalanche Features of Dune Slip Face Seen in MOC Image R06-00380: PSP_006899_1330 PSP_006965_1330 (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 | -46.7 | 20.1 | 8.63 | -9.75 | 65.3 | 67.4 |
Basal Exposure of South Polar Layered Deposits: PSP_005379_1060 PSP_005893_1060 (Interval in Earth days: 40) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -74.0 | 131. | -5.2 | 20.22 | 62.0 | 68.6 |
Small Valley Delta in Crater Near Maja Valles: PSP_005926_1850 ESP_011279_1850 (Interval in Earth days: 417) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.925 | 301. | -8.3 | 17.11 | 36.4 | 55.6 |
Holden Crater Megabreccia: PSP_006690_1530 PSP_006980_1530 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -26.9 | 325. | -7.5 | 14.55 | 49.3 | 52.4 |
Unnamed Well-Preserved Crater in Cimmeria Terra: PSP_005286_1480 PSP_005576_1480 (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 | -31.5 | 140. | -27. | -1.66 | 36.8 | 36.4 |
Hummocky Terrain and Polygonal Textures Seen in MOC Image M03-04266: PSP_005827_1260 PSP_006605_1260 (Interval in Earth days: 61) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -53.8 | 130. | 7.49 | -8.36 | 52.4 | 66.5 |
Xanthe Terra Crater: PSP_006598_1780 ESP_033326_1780 (Interval in Earth days: 2083) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.16 | 313. | 2.29 | 24.68 | 37.1 | 37.0 |
Spider Evolution Unfrosted: PSP_004947_0930 PSP_005104_0930 (Interval in Earth days: 13) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.0 | 98.9 | -0.2 | 16.73 | 68.1 | 68.0 |
Surface Morphology: PSP_005935_2275 ESP_011855_2275 (Interval in Earth days: 462) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 46.90 | 49.0 | 0.36 | 19.26 | 61.4 | 73.1 |
Spallanzani Crater - Swirl Patterns in Lower Layers along Northern Margin: PSP_005565_1220 PSP_005842_1220 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -57.7 | 86.3 | -5.0 | -20.8 | 52.1 | 57.2 |
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