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.
| Dark Dune Field Topography in Bunge Crater: ESP_072374_1460 ESP_072440_1460 (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 | -33.4 | 311. | 11.1 | -11.4 | 70.3 | 71.2 |
| Polar Terrain Imaging: ESP_072320_2580 ESP_072557_2580 (Interval in Earth days: 19) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 78.07 | 320. | 6.58 | 23.26 | 68.8 | 71.5 |
| Stratigraphic Relations in Scalloped Terrain: ESP_072263_2280 ESP_071841_2280 (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 | 47.84 | 91.0 | 8.08 | 27.48 | 54.9 | 48.1 |
| Layered Butte near Mawrth Vallis: ESP_072096_2065 ESP_072162_2065 (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 | 26.02 | 335. | 4.81 | -17.0 | 50.6 | 53.0 |
| Crater in Arabia Terra: ESP_072398_2220 ESP_072464_2220 (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 | 41.47 | 6.12 | 8.82 | -8.40 | 55.0 | 57.3 |
| North Polar Layered Deposits Crater: ESP_072095_2600 ESP_072003_2600 (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 | 79.83 | 340. | 8.87 | -5.16 | 66.3 | 66.0 |
| Candidate ExoMars Landing Site in Oxia Planum: ESP_072307_1985 ESP_072241_1985 (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 | 18.32 | 335. | -8.7 | 14.63 | 53.7 | 51.3 |
| Rough Polar Terrain: ESP_072267_2575 ESP_072214_2575 (Interval in Earth days: 4) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 77.12 | 332. | -1.2 | 14.67 | 68.0 | 66.1 |
| Translucent Ice on Dunes South Site: ESP_072321_2550 ESP_072268_2550 (Interval in Earth days: 4) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 74.99 | 299. | -1.4 | 17.00 | 67.7 | 65.6 |
| Channel in Cydonia Mensae: ESP_072201_2140 ESP_072412_2140 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 33.59 | 347. | 2.53 | -10.0 | 51.9 | 55.3 |
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