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.
Streamlined Hills in the Western Charitum Montes: PSP_006902_1275 ESP_011398_1275 (Interval in Earth days: 350) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -52.1 | 301. | -7.0 | 7.062 | 70.2 | 70.9 |
Layers at the Head of Chasma Australe Exposed over 270 Degrees of Azimuth: PSP_004788_0945 PSP_005079_0945 (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 | -85.6 | 95.5 | 0 | -16.3 | 65.3 | 69.7 |
Tomini Crater Western Ejecta: PSP_005695_1965 PSP_005985_1965 (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 | 16.25 | 125. | -1.0 | 26.25 | 42.8 | 38.2 |
Mawrth Vallis Phillosilicate Layers: PSP_005819_2050 PSP_006742_2050 (Interval in Earth days: 72) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.68 | 339. | 3.35 | -7.74 | 46.6 | 40.7 |
Seasonal Monitoring: PSP_005340_0930 PSP_005523_0930 (Interval in Earth days: 14) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.0 | 170. | 0.24 | 20.31 | 72.8 | 73.3 |
Fresh Crater: PSP_005517_2240 PSP_005807_2240 (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 | 43.80 | 301. | -0.2 | 20.25 | 65.1 | 59.8 |
West Mareotis Tholus: PSP_006718_2160 ESP_011557_2160 (Interval in Earth days: 378) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.67 | 271. | 1.41 | -25.3 | 44.9 | 67.7 |
Possible Exposure of Polar Layered Deposits in Area Not Well Observed: PSP_004882_0880 PSP_004894_0920 (Interval in Earth days: 1) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -88.1 | 121. | 11.7 | 11.47 | 68.6 | 67.9 |
Gullies with Dark Channels on South-Facing Crater Slope: PSP_005194_1445 PSP_005471_1445 (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 | -35.0 | 130. | -2.9 | -27.7 | 35.7 | 39.1 |
Dune Source in Newton Crater: PSP_006866_1375 ESP_015964_1375 (Interval in Earth days: 709) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -42.1 | 201. | -6.2 | 21.12 | 62.2 | 65.1 |
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