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 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 |
| Morphologically Fresh Incision in Potentially Ice-Rich Mantling Deposit: ESP_090370_2225 ESP_090436_2225 (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 | 41.91 | 34.0 | -3.7 | -16.2 | 60.6 | 62.6 |
| Terrain around Crater in Terra Sabaea: ESP_090409_2165 ESP_090132_2165 (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 | 36.18 | 50.6 | -6.7 | 5.045 | 59.7 | 55.3 |
| Monitor Changes in Intracrater Mounds: ESP_090444_2195 ESP_090378_2195 (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 | 39.18 | 175. | -8.2 | 5.181 | 61.3 | 59.2 |
| Canyon Walls in Coprates Chasma: ESP_090558_1655 ESP_094131_1655 (Interval in Earth days: 279) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.0 | 306. | 13.1 | 4.739 | 58.4 | 35.2 |
| Light-Toned Exposures on Floor of Coprates Chasma: ESP_090413_1645 ESP_090136_1645 (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 | -15.3 | 307. | 4.12 | 18.86 | 60.0 | 60.1 |
| An Inverted Channel in Flammarion Crater: ESP_089631_2065 ESP_090330_2065 (Interval in Earth days: 54) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 26.02 | 48.9 | 5.65 | -12.0 | 49.6 | 57.2 |
| Deep in Valles Marineris: ESP_089134_1655 ESP_088633_1655 (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 | -14.3 | 303. | -5.3 | -18.1 | 64.4 | 65.7 |
| Landing Site Characterization for Possible Future Rotorcraft : ESP_090127_2185 ESP_089204_2185 (Interval in Earth days: 72) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 38.18 | 186. | 4.89 | -13.2 | 55.7 | 48.1 |
| Dune Interaction with Residual Polar Ice: ESP_089932_2600 ESP_090156_2600 (Interval in Earth days: 18) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 79.66 | 99.1 | -7.9 | 1.407 | 70.2 | 73.1 |
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