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.
| Layers along Graben Wall of Arsia Mons Flank: ESP_077124_1725 ESP_077058_1725 (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 | -7.48 | 236. | -8.9 | 5.849 | 40.9 | 39.1 |
| Lava in Kasei Valles: ESP_077122_2025 ESP_077399_2025 (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 | 22.09 | 286. | -4.9 | 5.772 | 41.7 | 40.4 |
| Hydrated Materials in Columbus Crater: ESP_077218_1505 ESP_077640_1505 (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 | -29.2 | 193. | 0 | 23.47 | 51.7 | 56.7 |
| Streamlined Landforms adjacent to Shalbatana Vallis: ESP_077332_1895 ESP_078255_1895 (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 | 9.454 | 317. | -4.1 | 4.45 | 39.7 | 45.0 |
| Glacial (Ice) or Lava Flow?: ESP_076502_2100 ESP_077333_2100 (Interval in Earth days: 65) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 29.66 | 285. | 5.10 | 15.32 | 49.4 | 42.1 |
| Channel in Terra Cimmeria: ESP_077481_1415 ESP_086355_1415 (Interval in Earth days: 692) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.4 | 217. | 6.91 | 28.75 | 61.4 | 60.7 |
| Overlapping Landslides in Crater in Margaritifer Terra: ESP_077318_1920 ESP_076764_1920 (Interval in Earth days: 43) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 11.98 | 338. | 6.36 | -7.69 | 38.8 | 39.5 |
| Aram Chaos: ESP_077107_1820 ESP_077384_1820 (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 | 2.106 | 338. | -5.4 | 6.296 | 38.8 | 39.9 |
| Layers in West Melas Chasma: ESP_077109_1715 ESP_077043_1715 (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 | -8.53 | 285. | -7.5 | 6.737 | 41.0 | 39.2 |
| Slope Monitoring: ESP_077412_1665 ESP_094527_1665 (Interval in Earth days: 1333) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.4 | 297. | -4.0 | -21.2 | 46.2 | 40.6 |
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