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.
Potential Future Mars Landing Site in Noctis Labyrinthus: ESP_020089_1730 ESP_020511_1730 (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 | -6.93 | 261. | 4.03 | -15.6 | 55.3 | 55.8 |
Central Structure of Unnamed Crater near Thasis Region: ESP_020155_2130 ESP_020577_2130 (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 | 32.62 | 254. | 4.51 | -10.6 | 59.6 | 65.8 |
Phyllosilicates in Bedrock of Eastern Coprates Chasma: ESP_020259_1670 ESP_020681_1670 (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 | -12.9 | 301. | -2.7 | -19.5 | 56.2 | 55.4 |
Bedrock Layers Exposed in West Proctor Crater: ESP_020256_1320 ESP_020889_1320 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -47.6 | 28.2 | -5.3 | -20.9 | 67.7 | 58.9 |
Channels and Lava Flows: ESP_020261_2010 ESP_020683_2010 (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 | 20.66 | 241. | 6.17 | -9.72 | 57.1 | 61.6 |
Ulysses Fossae Region Grabens: ESP_020314_1935 ESP_020815_1935 (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 | 13.21 | 236. | -1.2 | 20.75 | 56.5 | 57.1 |
Spiders in Variety of Terrains: ESP_020229_0930 ESP_020230_0930 (Interval in Earth days: 0) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.0 | 86.4 | 9.23 | -2.36 | 88.6 | 89.9 |
Flow Structures in Noctis Region Trough: ESP_020313_1720 ESP_020735_1720 (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 | -8.08 | 265. | 4.07 | -12.9 | 54.9 | 54.8 |
Wrinkle Ridges in East Meridiani Planum: ESP_020138_1845 ESP_020283_1845 (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 | 4.462 | 2.88 | -6.0 | 7.354 | 55.3 | 54.6 |
Very Fresh Northern Plains 6-Kilometer Diameter Crater: ESP_020156_2235 ESP_028714_2235 (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 | 43.24 | 225. | -1.5 | 8.405 | 64.1 | 58.9 |
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