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.
| Possible Vent in Young Lava Flows in Elysium Region: ESP_089244_2090 ESP_089534_2090 (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 | 28.68 | 174. | 4.31 | 28.13 | 47.1 | 46.6 |
| Light-Toned Exposures in Capri Chasma: ESP_089582_1665 ESP_089437_1665 (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 | -13.1 | 312. | -0.7 | -17.4 | 62.4 | 64.0 |
| Positive Relief Material in Association with Osuga Valles Depression: ESP_089397_1655 ESP_089542_1655 (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 | -14.5 | 323. | -1.7 | 14.98 | 63.7 | 62.2 |
| Valley Attached to Northern Mid-Latitude Crater: ESP_089316_2135 ESP_089461_2135 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 33.34 | 7.71 | 5.13 | 17.17 | 47.2 | 47.2 |
| Light-Toned Mesas in Arcadia Planitia: ESP_089560_2260 ESP_089336_2260 (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 | 45.44 | 183. | 12.9 | -21.3 | 49.9 | 50.8 |
| Large Crater on Slope of Layered Deposits: ESP_089517_1735 ESP_089095_1735 (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 | -6.23 | 287. | -20. | -5.59 | 60.6 | 59.8 |
| Dune Interaction with Residual Polar Ice: ESP_089273_2595 ESP_089365_2595 (Interval in Earth days: 7) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 79.28 | 88.0 | -3.9 | 11.81 | 61.5 | 61.4 |
| Deposit in Small Northern Mid-Latitude Crater: ESP_089527_2115 ESP_089672_2115 (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 | 30.99 | 7.69 | 3.64 | 17.38 | 48.9 | 48.8 |
| Megadunes in Hyperborei Cavi: ESP_089212_2620 ESP_089238_2620 (Interval in Earth days: 2) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 82.03 | 312. | -8.3 | 5.626 | 62.8 | 62.2 |
| Possible Sulfate-Rich Deposit: ESP_089319_1730 ESP_089741_1730 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.16 | 291. | 5.45 | -5.79 | 59.4 | 59.6 |
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