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.
Light-Toned Layering along Plains Adjacent to Melas Chasma: PSP_005030_1685 ESP_012427_1685 (Interval in Earth days: 576) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.2 | 284. | 3.48 | -15.1 | 35.7 | 53.6 |
Basal Exposure of South Polar Layered Deposits: PSP_005089_1040 PSP_005313_1040 (Interval in Earth days: 18) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -75.8 | 131. | -6.9 | 7.077 | 60.1 | 61.9 |
Young Double-Layer Ejecta Crater: PSP_006816_2120 PSP_007027_2120 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 31.47 | 116. | 5.98 | -4.03 | 42.0 | 41.9 |
Light-Toned Layering on Plains Next to Ganges Chasma: PSP_005161_1720 ESP_016237_1720 (Interval in Earth days: 863) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.14 | 307. | 6.27 | -10.6 | 35.3 | 48.9 |
Ridges in Nili Fossae Phyllosilicates: PSP_005855_2020 PSP_006712_2020 (Interval in Earth days: 67) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.80 | 77.1 | -2.4 | 7.233 | 44.7 | 38.7 |
Light-Toned Layering in Plains South of Melas Chasma: PSP_006230_1690 ESP_012348_1690 (Interval in Earth days: 477) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -10.8 | 282. | 0 | -25.4 | 35.7 | 55.3 |
Fresh Impact Crater: PSP_005837_1965 PSP_005903_1965 (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 | 16.41 | 209. | -7.9 | -26.4 | 42.0 | 42.9 |
Fresh Pit Crater on Arsia Mons: PSP_004913_1735 PSP_005836_1735 (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 | -6.31 | 239. | -8.9 | 1.393 | 39.5 | 33.4 |
Alcove in West Hellas Region: PSP_006753_1425 PSP_010814_1425 (Interval in Earth days: 317) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.0 | 45.9 | 0 | -22.6 | 56.4 | 72.8 |
East Candor Region: PSP_004410_1735 ESP_012229_1735 (Interval in Earth days: 609) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.22 | 290. | 0.51 | -28.0 | 44.7 | 57.4 |
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