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.
| Layered Mound near Mawrth Vallis: ESP_090359_2045 ESP_090425_2045 (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 | 24.02 | 335. | 8.76 | -7.68 | 55.6 | 57.6 |
| 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 |
| Flow Obstacle in Lobate Debris Apron: ESP_090608_2215 ESP_090107_2215 (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 | 40.89 | 11.8 | 27.4 | 9.221 | 61.0 | 55.7 |
| Vent East of Ascraeus Mons: ESP_090375_1925 ESP_090520_1925 (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 | 12.13 | 261. | -5.8 | 10.07 | 56.2 | 55.7 |
| 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 |
| 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 |
| 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 |
| Terrain Northeast of Chryse Planitia: ESP_090214_2200 ESP_090491_2200 (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 | 39.48 | 332. | -3.6 | -16.1 | 57.8 | 62.7 |
| Mottled Ridged Terrain: ESP_090266_1840 ESP_090688_1840 (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 | 3.703 | 357. | -1.8 | -24.6 | 56.2 | 59.2 |
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