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.
| Eastern Discontinuous Ejecta and Rays of Tomini Crater : ESP_044146_1965 ESP_043790_1965 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 16.22 | 126. | 3.15 | -13.6 | 43.2 | 43.9 |
| Summit of One of Cerberus Tholi : ESP_044039_1850 ESP_044184_1850 (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 | 4.872 | 169. | -2.2 | 17.44 | 48.7 | 47.5 |
| Gullies in Northern Mid-Latitude Crater : ESP_044122_2335 ESP_051071_2335 (Interval in Earth days: 541) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 52.97 | 57.4 | -8.5 | 4.472 | 43.1 | 51.1 |
| Mini Cinder Cones in Aetheria Region : ESP_043896_2055 ESP_044885_2055 (Interval in Earth days: 77) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 25.07 | 110. | -3.2 | 19.02 | 40.7 | 40.2 |
| Streamlined Features and Small Channels adjacent to Ravi Vallis : ESP_043994_1800 ESP_044139_1800 (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 | -0.09 | 318. | -9.2 | 11.23 | 51.8 | 50.7 |
| Channels on Alba Patera : ESP_044115_2270 ESP_044194_2270 (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 | 46.73 | 248. | 1.66 | 25.66 | 40.5 | 38.4 |
| Nili Patera Dunes : ESP_043990_1890 ESP_044346_1890 (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 | 8.769 | 67.1 | -12. | 7.288 | 47.4 | 46.4 |
| Light-Toned Ridges with Possible Mounds : ESP_043925_2310 ESP_043635_2310 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 50.82 | 31.0 | 22.7 | 3.014 | 39.8 | 42.2 |
| Pit Near Elysium Mons : ESP_043974_2090 ESP_078591_2090 (Interval in Earth days: 2698) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 28.58 | 139. | 6.47 | 21.08 | 39.4 | 41.0 |
| Northern Arabia Terra Deposits : ESP_044124_2185 ESP_044058_2185 (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 | 38.21 | 3.93 | 2.19 | 16.92 | 39.4 | 38.0 |
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