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.
| Edge of South Polar Residual Cap: ESP_067636_0920 ESP_058933_0920 (Interval in Earth days: 678) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -88.1 | 45.8 | 29.4 | 19.28 | 80.4 | 82.9 |
| Hydaspis Chaos: ESP_067374_1825 ESP_074852_1825 (Interval in Earth days: 582) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.223 | 335. | -5.0 | -17.0 | 41.3 | 52.8 |
| Layering in Argyre Planitia: ESP_067573_1245 ESP_066966_1245 (Interval in Earth days: 47) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -55.2 | 314. | -0.7 | 15.46 | 56.9 | 47.7 |
| Fractures in Chryse Planitia: ESP_067348_1980 ESP_067546_1980 (Interval in Earth days: 15) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.85 | 321. | 7.95 | -17.0 | 47.8 | 47.9 |
| Searching for Slope Features: ESP_067410_1515 ESP_076853_1515 (Interval in Earth days: 735) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -28.1 | 76.1 | 5.88 | -23.1 | 40.2 | 47.0 |
| Valley-Inverted Channel Transition in Arabia Terra: ESP_067636_1875 ESP_067504_1875 (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 | 7.578 | 26.2 | -1.2 | 15.33 | 42.0 | 41.2 |
| Gullies on Mound in Nereidum Montes: ESP_067467_1350 ESP_067876_1350 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -44.5 | 324. | -4.3 | 8.455 | 48.9 | 54.5 |
| Candidate ExoMars Landing Site in Oxia Planum: ESP_067519_1980 ESP_076830_1980 (Interval in Earth days: 725) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.84 | 336. | 8.05 | -2.37 | 46.3 | 40.9 |
| South Polar Residual Cap: ESP_067611_0910 ESP_067467_0910 (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 | -88.9 | 17.0 | 28.7 | 23.99 | 80.6 | 78.8 |
| Eroded Crater with Eroded Floor in Hellas Region: ESP_067435_1385 ESP_076680_1385 (Interval in Earth days: 721) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -40.9 | 116. | -2.8 | 6.995 | 46.5 | 49.9 |
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