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.
Geometry of Ramparts for Crater in High Southern Latitudes: PSP_007800_1365 PSP_009593_1365 (Interval in Earth days: 139) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -43.3 | 258. | -5.1 | 7.815 | 76.5 | 83.0 |
Russell Crater Dunes: PSP_007018_1255 PSP_007229_1255 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -54.2 | 12.9 | 3.27 | -5.25 | 73.2 | 77.0 |
Northern Plains with Mounds and Filled Crater: PSP_007738_2480 PSP_007804_2480 (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 | 67.79 | 132. | 4.04 | -4.67 | 54.6 | 54.7 |
Central Peak of Large 40-Kilometer Diameter Crater: PSP_007592_1995 ESP_045595_1995 (Interval in Earth days: 2961) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 19.25 | 169. | -0.9 | 19.06 | 40.8 | 43.5 |
Eroded High-Latitude Mantle: PSP_007159_1405 PSP_007515_1405 (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 | -39.4 | 120. | 6.69 | -4.42 | 64.2 | 69.9 |
Pits at the Head of the Hephaestus Fossae: PSP_007264_1975 PSP_007554_1975 (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 | 17.42 | 127. | -7.3 | 5.253 | 40.1 | 40.3 |
Fan in Aeolis Region: PSP_007975_1755 PSP_009623_1755 (Interval in Earth days: 129) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.65 | 154. | -4.9 | 5.617 | 52.4 | 57.8 |
Mesas in Huo Hsing Vallis: PSP_007688_2075 PSP_008690_2075 (Interval in Earth days: 78) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 27.10 | 66.7 | 5.61 | -11.4 | 40.1 | 43.9 |
Layering in Eastern Central Peak of Oudemans Crater: PSP_007193_1700 PSP_008195_1700 (Interval in Earth days: 79) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.89 | 268. | 4.49 | -6.29 | 46.3 | 57.2 |
Central Peak of Fesenkov Crater: PSP_007931_2020 ESP_024585_2020 (Interval in Earth days: 1298) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.68 | 273. | -8.3 | -25.5 | 42.4 | 39.6 |
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