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.
| 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 |
| 5 Kilometer Diameter Impact Crater Northwest of Mojave Crater: ESP_013968_1890 ESP_014390_1890 (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 | 8.866 | 328. | 6.90 | -3.58 | 44.6 | 40.6 |
| South Polar Layered Deposits Exposed in Ultimum Chasma: ESP_013619_0990 ESP_013672_0990 (Interval in Earth days: 4) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -80.8 | 151. | 18.0 | 4.365 | 60.2 | 61.5 |
| Possible Blocky Deposit in Melas Chasma: ESP_013508_1665 ESP_014141_1665 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.2 | 289. | 6.08 | -18.0 | 39.2 | 35.6 |
| Nili Fossae-NE Syrtis Phyllosilicate-Sulfate Stratigraphy: ESP_013041_1975 ESP_030025_1975 (Interval in Earth days: 1324) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.42 | 76.9 | -3.2 | 12.81 | 61.2 | 60.4 |
| Upper Reach of Mamers Valles: ESP_013254_2115 ESP_021825_2115 (Interval in Earth days: 668) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 31.09 | 18.9 | 5.76 | 15.24 | 68.5 | 68.2 |
| Layers on Columbus Crater Wall: ESP_014105_1495 ESP_014382_1495 (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 | -30.0 | 193. | -0.6 | -23.8 | 34.9 | 38.0 |
| Alcove in East Candor Chasma Layered Deposits: ESP_012809_1725 ESP_013310_1725 (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 | -7.44 | 293. | -2.1 | 22.37 | 50.2 | 42.7 |
| Pit Crater Chain Southwest of Arsia Mons: ESP_014077_1660 ESP_058186_1660 (Interval in Earth days: 3437) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.9 | 236. | -3.3 | 8.798 | 34.6 | 29.8 |
| Exposure of Thick Layered Deposits in Hebes Chasma: ESP_013205_1790 ESP_021565_1790 (Interval in Earth days: 651) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.82 | 283. | -25. | -3.43 | 50.5 | 51.4 |
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