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.
| South Polar Residual Cap Deposits: ESP_048477_0930 ESP_048702_0930 (Interval in Earth days: 18) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -86.7 | 16.3 | 5.97 | -4.05 | 64.4 | 66.0 |
| Gullies in Crater in Aonia Terra : ESP_048256_1225 ESP_048546_1225 (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 | -57.0 | 250. | -6.2 | 3.654 | 46.5 | 43.7 |
| Western Ejecta and Rays of Gasa Crater : ESP_048458_1440 ESP_057346_1440 (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 | -35.7 | 129. | 4.67 | -24.4 | 36.4 | 38.1 |
| Li Fan Crater Fan Landforms : ESP_048508_1330 ESP_048798_1330 (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 | -46.7 | 206. | -5.5 | 11.90 | 39.6 | 37.0 |
| The Coolest Landscape on Mars (or Earth): ESP_047304_0930 ESP_047237_0930 (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 | -86.7 | 16.3 | -0.0 | 16.3 | 77.5 | 77.1 |
| Hellas Planitia Western Rim : ESP_048171_1320 ESP_048962_1320 (Interval in Earth days: 62) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -47.5 | 48.6 | 0 | 18.61 | 43.0 | 36.8 |
| Streamlined Island in Outflow Channel Located in Ares Vallis : ESP_048055_1960 ESP_048345_1960 (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 | 16.05 | 330. | -28. | -14.9 | 60.1 | 57.5 |
| Light-Toned Fragments in Linear Depressions : ESP_047965_1720 ESP_048967_1720 (Interval in Earth days: 79) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.92 | 267. | 0 | 13.75 | 46.4 | 34.9 |
| USGS Dune Database Entry Number 3470-331: ESP_048160_1465 ESP_048806_1465 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -33.1 | 346. | -3.6 | 6.396 | 40.3 | 32.9 |
| Cratered Cones and Ridges in Isidis Planitia : ESP_047998_1975 ESP_048565_1975 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.24 | 83.4 | 0 | -22.7 | 59.1 | 57.0 |
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