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.
Possible Monohydrated Sulfate-Rich Terrain in Columbus Crater: ESP_014039_1510 ESP_021832_1510 (Interval in Earth days: 607) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -28.7 | 194. | 7.74 | 26.60 | 33.9 | 38.3 |
Raga Crater: ESP_014011_1315 ESP_014288_1315 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -48.1 | 242. | 1.60 | -18.1 | 41.9 | 45.6 |
Interesting Contrasts in Gully Morphology: ESP_014104_1360 ESP_021686_1360 (Interval in Earth days: 591) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -43.8 | 222. | 3.50 | 25.74 | 40.1 | 42.0 |
Gullies: ESP_012722_1400 ESP_012867_1400 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.6 | 153. | -6.2 | 7.111 | 47.5 | 44.4 |
Relatively Fresh 1-Kilometer Diameter Crater in South Polar Region : ESP_013699_1055 ESP_013923_1055 (Interval in Earth days: 18) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -74.1 | 130. | -4.9 | 10.22 | 57.2 | 58.2 |
5 Kilometer Diameter Impact Crater Northwest of Mojave Crater: ESP_013968_1890 ESP_014390_1890 (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 | 8.866 | 328. | 6.90 | -3.58 | 44.6 | 40.6 |
Alcove in East Candor Chasma Layered Deposits: ESP_012809_1725 ESP_013310_1725 (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 | -7.44 | 293. | -2.1 | 22.37 | 50.2 | 42.7 |
Floor of Mawrth Vallis: ESP_014007_2030 ESP_022578_2030 (Interval in Earth days: 668) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 22.98 | 341. | 9.10 | 25.33 | 53.5 | 54.6 |
Possible Blocky Deposit in Melas Chasma: ESP_013508_1665 ESP_014141_1665 (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 | -13.2 | 289. | 6.08 | -18.0 | 39.2 | 35.6 |
Layers in Spallanzani Crater: ESP_013041_1215 ESP_013120_1215 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -58.1 | 86.8 | 5.04 | 26.10 | 48.1 | 45.8 |
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