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.
| Sample of Aprons around Massifs in Erebus Montes: ESP_090404_2185 ESP_090338_2185 (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 | 38.34 | 187. | -8.8 | 5.02 | 60.5 | 58.4 |
| Okavango Valles: ESP_090595_2185 ESP_090516_2185 (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 | 38.24 | 8.82 | 17.2 | -4.81 | 60.9 | 61.7 |
| Survey of Terrain around Ice-Exposing Crater: ESP_090417_2195 ESP_090628_2195 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 39.25 | 190. | 8.58 | -5.83 | 59.5 | 63.6 |
| Kasei Valles Dissected Alluvial Fans: ESP_090400_2060 ESP_090466_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 | 25.88 | 297. | -0.8 | -16.8 | 57.0 | 59.0 |
| Potential Landing Sites in Capri Chasma: ESP_090426_1665 ESP_090070_1665 (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 | -13.4 | 311. | 4.49 | -21.8 | 59.4 | 62.7 |
| Bench in Samara Valles: ESP_090425_1545 ESP_090715_1545 (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 | -25.0 | 340. | 3.09 | 12.71 | 63.4 | 60.4 |
| Alluvial Fan in Coprates Catena Trough: ESP_090308_1650 ESP_090453_1650 (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 | -14.6 | 294. | -16. | 8.504 | 61.8 | 59.4 |
| Inverted Channels or Possible Eskers in Basin in Northwest Arabia Terra: ESP_090371_2150 ESP_090437_2150 (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 | 34.65 | 6.53 | 8.59 | -5.85 | 57.7 | 59.7 |
| Small Delta or Fan: ESP_090395_2065 ESP_082088_2065 (Interval in Earth days: 647) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 26.38 | 74.4 | -11. | 7.284 | 57.8 | 62.6 |
| Inverted Dendritic Channels in Noachis Terra Crater: ESP_090370_1555 ESP_090581_1555 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -24.1 | 41.6 | 6.89 | -5.62 | 63.2 | 62.6 |
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