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.
| Dune Interaction with Residual Polar Ice: ESP_089589_2600 ESP_089470_2600 (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 | 79.63 | 97.9 | 1.02 | 16.15 | 64.9 | 62.5 |
| Ismenius Cavus Channel: ESP_089342_2145 ESP_090252_2145 (Interval in Earth days: 71) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 34.01 | 17.7 | 5.30 | -17.5 | 47.4 | 58.3 |
| Fan-Shaped Deposit in Arcadia Planitia: ESP_089428_2200 ESP_089494_2200 (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 | 39.86 | 188. | 6.33 | -9.62 | 48.3 | 50.2 |
| Layering in Southern Lucus Planum: ESP_089336_1720 ESP_089481_1720 (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 | -7.84 | 187. | 4.06 | 19.82 | 59.8 | 58.4 |
| Sample of Scalloped Terrain West of Erebus Montes: ESP_089349_2195 ESP_089072_2195 (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 | 39.37 | 187. | -8.3 | 14.20 | 48.9 | 44.9 |
| 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 |
| 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 |
| Features around Crater in Arabia Terra: ESP_089592_2190 ESP_089104_2190 (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 | 38.44 | 34.3 | -16. | 10.19 | 51.6 | 45.4 |
| Potential Compound Dune: ESP_089573_2610 ESP_089389_2610 (Interval in Earth days: 14) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 80.87 | 160. | 19.2 | -5.86 | 64.3 | 63.7 |
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