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.
| Proposed Site for Future Exploration in Capri Chasma: ESP_085811_1665 ESP_085468_1665 (Interval in Earth days: 26) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.3 | 312. | -7.7 | 11.52 | 41.0 | 36.0 |
| Small Delta or Fan: ESP_085751_1725 ESP_085962_1725 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.46 | 147. | 8.32 | -7.47 | 37.5 | 40.7 |
| Kasei Valles Lava: ESP_085825_1965 ESP_085614_1965 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 16.14 | 285. | 4.28 | -6.99 | 39.1 | 40.5 |
| Layering in Lucus Planum: ESP_085895_1715 ESP_086330_1715 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.38 | 177. | -7.9 | 12.91 | 40.3 | 43.6 |
| Raised Circular Feature: ESP_085811_2210 ESP_086246_2210 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.81 | 305. | -6.0 | 6.055 | 51.8 | 47.1 |
| Transect of Ladon Valles: ESP_085441_1560 ESP_085507_1560 (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 | -23.7 | 330. | 9.97 | -6.87 | 39.3 | 41.3 |
| Margin of Smooth Lobate Deposit in Nereidum Montes: ESP_085626_1410 ESP_085758_1410 (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 | -38.8 | 322. | 16.8 | -8.36 | 49.8 | 53.5 |
| Pitted Cones near Crater: ESP_085515_2060 ESP_085449_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 | 25.75 | 105. | 1.87 | 16.40 | 45.1 | 44.7 |
| Curved Channel near Crater Rim: ESP_085495_2165 ESP_085983_2165 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.91 | 289. | -1.3 | -16.0 | 51.8 | 48.1 |
| Landforms above Subsurface Radar Observations of South Polar Cap: ESP_085475_1065 ESP_085554_1065 (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 | -73.5 | 135. | -4.3 | 10.13 | 73.9 | 74.5 |
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