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 ExoMars Landing Site: ESP_037361_1920 ESP_045181_1920 (Interval in Earth days: 610) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 11.88 | 313. | -10. | 4.934 | 55.3 | 45.4 |
| Candidate Landing Site for 2020 Mission in Jezero Crater: ESP_037396_1985 ESP_042315_1985 (Interval in Earth days: 383) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.45 | 77.3 | -8.0 | -27.9 | 55.3 | 41.1 |
| Candidate Landing Site for 2020 Mission in Oyama Crater: ESP_037505_2035 ESP_037993_2035 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.46 | 340. | 1.30 | -13.3 | 55.9 | 62.0 |
| A New Impact Crater near NASA's InSight Landing Region: ESP_037328_1845 ESP_037684_1845 (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 | 4.338 | 135. | -5.5 | 13.50 | 55.6 | 55.1 |
| Strange Cones and Flows: ESP_037222_1820 ESP_042141_1820 (Interval in Earth days: 384) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 1.807 | 147. | 18.1 | 0.765 | 53.9 | 38.8 |
| Candidate Landing Site for 2020 Mission: ESP_037151_1675 ESP_037507_1675 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.2 | 290. | -14. | 1.067 | 60.9 | 58.8 |
| Sinuous Ridge System in Intercrater Terrain: ESP_037050_1625 ESP_037195_1625 (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 | -17.1 | 167. | -6.8 | 7.753 | 62.7 | 61.1 |
| Crater Floor with Ridges in Central Arabia Terra: ESP_036857_1915 ESP_037701_1915 (Interval in Earth days: 66) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 11.28 | 32.8 | 3.8 | -15.5 | 51.8 | 57.7 |
| Fractured Ground in Northeast Syrtis Major Planum: ESP_036829_1980 ESP_037040_1980 (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 | 17.56 | 76.8 | -0.6 | -11.2 | 50.8 | 53.0 |
| Light-Toned Layered Deposits in Noctis Labyrinthus: ESP_036875_1695 ESP_037297_1695 (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 | -10.3 | 264. | 0 | -17.9 | 59.6 | 60.1 |
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