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.
| Inverted Channel in Noachis Terra Displaying Morphological Change: ESP_085572_1440 ESP_085506_1440 (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 | -35.7 | 358. | -7.2 | 7.596 | 48.5 | 46.6 |
| Northern Terra Cimmeria: ESP_085541_1740 ESP_086319_1740 (Interval in Earth days: 61) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.31 | 119. | 3.84 | -8.46 | 36.1 | 44.2 |
| Unusual Textured Cratered Floor with Outlet Channel in Southern Highlands: ESP_085401_1480 ESP_085744_1480 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -31.5 | 344. | -7.2 | -23.1 | 43.6 | 49.8 |
| Margin of Athabasca Valles Lava: ESP_085672_1835 ESP_085738_1835 (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 | 3.686 | 142. | 7.88 | -7.30 | 36.3 | 37.7 |
| Triangular Faceted Spurs in East Candor Chasma: ESP_085693_1740 ESP_085838_1740 (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 | -6.03 | 291. | -3.9 | 20.84 | 37.7 | 36.9 |
| Sand Sheet Activity Monitoring: ESP_085641_1275 ESP_085786_1275 (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 | -52.0 | 276. | 3.68 | 24.67 | 60.0 | 61.3 |
| Crater with Steep Slopes: ESP_085136_1375 ESP_085690_1375 (Interval in Earth days: 43) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -42.0 | 18.7 | 7.38 | -8.12 | 45.0 | 54.5 |
| Lighter-Toned Deposits in Young Crater: ESP_085271_1870 ESP_085337_1870 (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 | 7.156 | 287. | -1.6 | -20.0 | 38.2 | 39.4 |
| Tempe Fossae: ESP_085099_2280 ESP_085231_2280 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 47.56 | 295. | 15.0 | -10.4 | 64.8 | 64.2 |
| Streamlined Form and Hill in Marte Vallis: ESP_085156_1980 ESP_085433_1980 (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 | 17.73 | 185. | 7.29 | -6.33 | 43.5 | 42.2 |
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