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.
South Polar Layered Deposits Exposed in Promethei Lingula: ESP_013714_0970 ESP_013687_0970 (Interval in Earth days: 3) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -82.8 | 116. | -28. | -8.52 | 66.4 | 64.2 |
Layering in Crater: ESP_013057_1825 ESP_013769_1825 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.613 | 1.41 | 3.63 | 16.95 | 51.9 | 42.7 |
Valley with Central Ridge Located North of Schiaparelli Crater: ESP_014164_1870 ESP_020388_1870 (Interval in Earth days: 485) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 6.827 | 16.4 | 19.0 | -0.77 | 40.3 | 55.8 |
Well-Preserved Large Crater West of Elysium Region: ESP_013567_2035 ESP_021571_2035 (Interval in Earth days: 624) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.31 | 114. | 5.79 | 18.66 | 59.6 | 63.4 |
Lava Flow Margin in Echus Chasma: ESP_013271_1810 ESP_013693_1810 (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 | 1.211 | 279. | 2.08 | -12.7 | 48.9 | 44.8 |
Aram Chaos: ESP_013783_1820 ESP_022486_1820 (Interval in Earth days: 678) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.171 | 339. | 7.62 | -21.2 | 42.9 | 44.4 |
Exposure of South Polar Layered Deposits with Minor Faulting: ESP_012855_1065 ESP_012723_1065 (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 | -73.2 | 132. | -7.1 | 7.21 | 58.4 | 58.8 |
Gullies in Crater North of Gorgonum Chaos: ESP_013169_1450 ESP_013314_1450 (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 | -34.7 | 189. | -4.4 | 7.868 | 41.0 | 38.5 |
Central Uplift of Well-Exposed Taytay Crater : ESP_012794_1875 ESP_012939_1875 (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 | 7.398 | 340. | 8.24 | 23.49 | 56.4 | 54.2 |
Light-Toned Outcrop in Lower Coprates Chasma Wall: ESP_013231_1690 ESP_013732_1690 (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 | -10.9 | 292. | 1.57 | 23.81 | 43.7 | 36.2 |
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