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.
| Fresh 3-Kilometer Diameter Crater Near Hellas Planitia: ESP_016681_1575 ESP_017393_1575 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -22.1 | 67.3 | -6.1 | 7.478 | 62.0 | 66.5 |
| Field of Small Volcanoes Northeast of Ascraeus Mons: ESP_016832_1885 ESP_017254_1885 (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 | 8.580 | 259. | 8.08 | -10.9 | 44.8 | 48.3 |
| Very Well-Preserved 9-Kilometer Diameter Impact Crater: ESP_016490_2315 ESP_016780_2315 (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 | 51.39 | 234. | -21. | -2.88 | 48.2 | 45.3 |
| Aram Chaos: ESP_016750_1830 ESP_017172_1830 (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 | 2.769 | 339. | 3.01 | -13.3 | 47.2 | 51.0 |
| Remnant Mantiling Deposit in Millochau Crater: ESP_016377_1585 ESP_017010_1585 (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 | -21.2 | 85.4 | 7.40 | -9.53 | 57.1 | 64.5 |
| Source Region for Branch of Auqakuh Vallis: ESP_016826_2080 ESP_016971_2080 (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 | 27.47 | 62.7 | -7.7 | 5.246 | 41.4 | 40.6 |
| Northern Plains West of Erebus Montes: ESP_016650_2205 ESP_035427_2205 (Interval in Earth days: 1464) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.26 | 185. | -1.2 | 27.98 | 42.1 | 39.3 |
| Well-Preserved Crater in Margaritifer Terra: ESP_016407_1675 ESP_016763_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 | -12.5 | 345. | -0.5 | 12.61 | 52.5 | 55.3 |
| Possible Phyllosilicates in Her Desher Vallis: ESP_016527_1550 ESP_025032_1550 (Interval in Earth days: 663) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -24.8 | 311. | -6.8 | 7.004 | 62.1 | 56.3 |
| Layered Deposits along Floor of Melas Chasma: ESP_016673_1700 ESP_017952_1700 (Interval in Earth days: 100) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.67 | 284. | -5.2 | 5.092 | 53.8 | 59.7 |
Page 689 of 878 (8,772 images) | |||||