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.
| Candidate Landing Site for 2020 Mission in Melas Chasma : ESP_044180_1700 ESP_044325_1700 (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 | -9.80 | 283. | -24. | -4.34 | 59.1 | 57.9 |
| Channel Entering Crater in Sirenum Fossae : ESP_044156_1560 ESP_044512_1560 (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 | -23.6 | 220. | -23. | -2.85 | 68.4 | 67.3 |
| Mesa with Ciruclar and Arcuate Scarp Elements : ESP_044114_2315 ESP_044734_2315 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 51.21 | 274. | 1.21 | -28.9 | 41.7 | 45.8 |
| 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 |
| Landforms in the Nili Fossae Region : ESP_043871_1995 ESP_045058_1995 (Interval in Earth days: 93) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 19.06 | 72.9 | 5.19 | -23.1 | 41.6 | 45.4 |
| 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 |
| 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 |
| Small Crater in Tempe Terra with Gullies and Outflow Channel : ESP_043824_2180 ESP_044101_2180 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 37.54 | 273. | 5.73 | -11.4 | 38.9 | 40.5 |
| 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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