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.
| Well-Preserved 5-Kilometer Diameter Impact Crater: ESP_018478_2150 ESP_018979_2150 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 34.78 | 318. | -3.5 | 13.05 | 44.5 | 46.3 |
| Cones at Edge of North Polar Layered Deposits: ESP_018387_2600 ESP_026576_2600 (Interval in Earth days: 638) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 79.99 | 270. | -8.4 | -24.5 | 59.2 | 58.2 |
| Valley in Libya Montes: ESP_018223_1830 ESP_018368_1830 (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 | 2.730 | 84.7 | -6.4 | 9.665 | 53.4 | 52.3 |
| Candor Chasma: ESP_018387_1730 ESP_019666_1730 (Interval in Earth days: 99) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.02 | 288. | -4.5 | 13.11 | 58.7 | 55.3 |
| Rounded Mounds in Cydonia Region: ESP_018411_2235 ESP_018134_2235 (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 | 43.13 | 346. | -1.5 | 17.83 | 44.5 | 41.4 |
| Cones at Edge of North Polar Layered Deposits: ESP_018109_2580 ESP_026654_2580 (Interval in Earth days: 666) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 77.90 | 298. | -0.4 | -19.2 | 56.1 | 56.6 |
| Bull's-Eye Impact Crater: ESP_018522_2270 ESP_019010_2270 (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 | 46.56 | 194. | 2.26 | -21.5 | 45.4 | 51.7 |
| Future Mars Landing Site in Acidalia Mensa: ESP_018161_2270 ESP_018227_2270 (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 | 46.68 | 331. | -1.6 | -15.5 | 43.8 | 45.4 |
| Future Mars Landing Site in Antoniadi Crater: ESP_018105_2045 ESP_018250_2045 (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 | 24.05 | 63.0 | -0.2 | 13.32 | 44.2 | 43.5 |
| Small Rayed Crater in Elysium Planitia: ESP_017785_1975 ESP_018418_1975 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.20 | 160. | 5.75 | -15.8 | 45.1 | 48.3 |
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