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.
| Head of Rille East of Hecates Tholus: ESP_012036_2125 ESP_012748_2125 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 32.12 | 152. | 1.95 | 14.72 | 69.1 | 71.0 |
| Light-Toned Outcrop in Hummock of Iani Chaos: ESP_012438_1795 ESP_012728_1795 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.68 | 342. | -3.8 | 23.07 | 55.8 | 51.8 |
| Fresh Crater with Lots of Gullies: ESP_011672_1395 ESP_011817_1395 (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 | -40.3 | 20.1 | -7.0 | 7.602 | 63.3 | 60.3 |
| East Portion of Flow in Harmakhis Vallis: ESP_012434_1420 ESP_012579_1420 (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 | -37.7 | 95.5 | 1.58 | 12.57 | 51.0 | 48.0 |
| Stepped Fan: ESP_011863_1715 ESP_012008_1715 (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 | -8.51 | 200. | 1.55 | 16.71 | 56.5 | 54.6 |
| Disrupted Terrain in Southern Elysium Planitia: ESP_012392_1800 ESP_025565_1800 (Interval in Earth days: 1026) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.09 | 159. | -17. | -8.18 | 57.3 | 48.1 |
| Central Uplift and Pitted and Ponded Material in Well-Preserved Crater: ESP_011761_1485 ESP_011827_1485 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -31.2 | 108. | -4.3 | -23.2 | 59.6 | 60.4 |
| Layered Material in Arabia Terra: ESP_012226_1815 ESP_012859_1815 (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 | 1.421 | 8.72 | 6.14 | -17.3 | 56.8 | 54.6 |
| Embayed Crater in Western Elysium Planitia: ESP_011720_1835 ESP_012353_1835 (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 | 3.484 | 142. | 7.82 | -9.32 | 57.5 | 58.2 |
| Eastern Half of Well-Preserved 7-Kilometer Diameter Gullied Crater: ESP_012483_1425 ESP_012338_1425 (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 | -37.2 | 198. | -5.3 | -17.7 | 50.7 | 53.8 |
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