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 |
Cerberus Fossae Region Seen in THEMIS Image: ESP_016651_1895 ESP_044026_1895 (Interval in Earth days: 2134) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.408 | 161. | 2.65 | 18.14 | 43.8 | 44.8 |
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 |
Very Recent Small Impact Crater: ESP_016630_1720 ESP_030291_1720 (Interval in Earth days: 1064) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.08 | 17.6 | -3.5 | 8.058 | 52.4 | 48.4 |
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 |
Columnar Jointing in West Wall of Crater in Marte Vallis: ESP_016360_2020 ESP_016505_2020 (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 | 21.55 | 184. | 7.23 | 21.49 | 39.4 | 38.5 |
Isolated Layered Mound in Trough Between Layered Benches in Terby Crater: ESP_016628_1520 ESP_016773_1520 (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 | -27.6 | 74.4 | 0.18 | 16.62 | 64.9 | 65.4 |
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 |
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