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.
| Mesa Stratigraphy at Terby Crater: ESP_085068_1525 ESP_085213_1525 (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 | -27.1 | 74.1 | -4.4 | 13.86 | 37.8 | 37.8 |
| Exposure of South Polar Layered Deposits: ESP_085009_0905 ESP_085037_0905 (Interval in Earth days: 2) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -89.5 | 289. | 29.6 | 26.87 | 77.2 | 78.0 |
| Impact Related Deposits and Flows near Hadriacus Mons: ESP_085107_1495 ESP_092926_1495 (Interval in Earth days: 610) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -30.3 | 89.4 | 0.42 | 20.13 | 39.1 | 35.2 |
| Dark Lanes in South Polar Residual Cap: ESP_085022_0905 ESP_076186_0905 (Interval in Earth days: 689) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -89.2 | 306. | 26.9 | 29.78 | 77.5 | 76.8 |
| Landforms above Subsurface Radar Observations of South Polar Cap: ESP_085104_0975 ESP_085012_0975 (Interval in Earth days: 7) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -82.1 | 188. | 7.05 | -7.33 | 73.9 | 73.3 |
| Sinuous Ridges on Both Sides of Scarp in Aeolis Planum: ESP_084920_1730 ESP_085065_1730 (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 | -6.73 | 151. | -1.5 | 13.33 | 35.5 | 34.1 |
| South Polar Residual Cap: ESP_084980_0915 ESP_067508_0915 (Interval in Earth days: 1361) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -88.3 | 340. | 25.6 | 18.92 | 75.9 | 79.5 |
| Landforms in Utopia Planitia: ESP_085146_2110 ESP_085423_2110 (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 | 30.77 | 96.2 | 7.62 | -4.77 | 52.0 | 49.5 |
| Channel Northeast of Hellas Planitia: ESP_084975_1630 ESP_092794_1630 (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 | -16.7 | 91.4 | 0 | 27.65 | 34.7 | 37.4 |
| Dunes in Terra Cimmeria: ESP_084986_1415 ESP_085342_1415 (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 | -38.2 | 154. | -1.9 | 14.25 | 41.6 | 45.1 |
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