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.
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 |
Possible Phyllosilicate-Rich Area in Syrtis Major: ESP_016628_2040 ESP_017340_2040 (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 | 23.69 | 68.6 | -7.2 | 6.233 | 41.2 | 42.0 |
Fretted Valley Outlet: ESP_016391_2195 ESP_016668_2195 (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 | 38.96 | 56.1 | -0.8 | -19.4 | 42.2 | 43.3 |
Deposits on the Floor of Palos Crater: ESP_016943_1775 ESP_017721_1775 (Interval in Earth days: 61) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.67 | 111. | 5.57 | -9.88 | 51.3 | 55.9 |
Candidate Landing Site in a Possible Salt Playa: ESP_016288_1745 ESP_016433_1745 (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 | -5.64 | 353. | 0.58 | 17.63 | 47.4 | 47.7 |
Exposure of Mid-Latitude Apron Interior by Younger Gully: ESP_015947_1370 ESP_051036_1370 (Interval in Earth days: 2734) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -42.5 | 308. | -3.0 | -16.8 | 66.5 | 62.9 |
Mounds on Hrad Vallis Mudflow: ESP_016256_2155 ESP_016322_2155 (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 | 35.06 | 142. | -2.8 | -19.2 | 41.7 | 43.0 |
Juventae Region Mound and Possible Sulfate-Rich Terrain: ESP_015934_1760 ESP_016646_1760 (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 | -3.74 | 298. | 0 | 21.43 | 42.9 | 48.4 |
Noachis Terra Sample: ESP_016182_1560 ESP_016815_1560 (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 | -23.5 | 9.41 | 6.53 | -7.78 | 56.2 | 64.3 |
Stratigraphic Relations in MOC Image M00-02426 in Sinus Meridiani: ESP_016169_1790 ESP_019637_1790 (Interval in Earth days: 270) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.77 | 1.73 | 4.18 | -16.4 | 43.8 | 56.0 |
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