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.
Alluvial Fans in Kasei Valles: ESP_085574_2030 ESP_085640_2030 (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 | 22.67 | 293. | 15.8 | 1.691 | 42.0 | 42.6 |
Triangular Faceted Spurs in East Candor Chasma: ESP_085693_1740 ESP_085838_1740 (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 | -6.03 | 291. | -3.9 | 20.84 | 37.7 | 36.9 |
Landforms above Subsurface Radar Observations of South Polar Cap: ESP_085526_1000 ESP_085513_1000 (Interval in Earth days: 1) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -79.7 | 185. | 8.77 | -3.25 | 79.0 | 79.5 |
Xanthe Dorsa: ESP_085335_2125 ESP_085480_2125 (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 | 32.46 | 337. | -1.4 | 19.20 | 51.4 | 48.4 |
Fissure in Athabasca Valles: ESP_085500_1900 ESP_085711_1900 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.733 | 156. | 1.29 | 15.59 | 38.1 | 36.6 |
Margin of Smooth Lobate Deposit in Nereidum Montes: ESP_085626_1410 ESP_085758_1410 (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 | -38.8 | 322. | 16.8 | -8.36 | 49.8 | 53.5 |
Ridge-Crater Relationships in Osuga Valles: ESP_085349_1650 ESP_085982_1650 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.7 | 321. | -4.2 | 3.855 | 36.6 | 42.7 |
Inverted Channel in Noachis Terra: ESP_085571_1600 ESP_085782_1600 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -19.9 | 23.0 | -4.5 | 12.69 | 40.3 | 41.8 |
Pitted Cones near Crater: ESP_085515_2060 ESP_085449_2060 (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 | 25.75 | 105. | 1.87 | 16.40 | 45.1 | 44.7 |
Large Isolated Landform at Chryse Planitia Margin: ESP_085402_1945 ESP_085547_1945 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 14.22 | 310. | 5.37 | 29.46 | 39.9 | 37.2 |
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