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.
| Characterize Possilbe Rotorcraft Landing Site: ESP_089283_2205 ESP_089362_2205 (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 | 39.97 | 189. | -7.1 | 19.14 | 48.3 | 46.5 |
| 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 |
| 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 |
| 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 |
| 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 |
| 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 |
| 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 |
| 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 |
| Skylight Candidate near Elysium Mons: ESP_089522_2090 ESP_089667_2090 (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 | 28.91 | 145. | -3.6 | 11.04 | 49.5 | 49.3 |
| Thermal Anomaly in Young Lava Flows of Elysium Region: ESP_089284_1970 ESP_089429_1970 (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 | 17.03 | 163. | 2.69 | 16.88 | 49.6 | 48.9 |
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