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.
Transverse Dunes West of Argyre Planitia: ESP_085825_1300 ESP_085759_1300 (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 | -49.8 | 294. | -2.2 | 12.44 | 61.9 | 59.9 |
Proposed Site for Future Exploration in Capri Chasma: ESP_085811_1665 ESP_085468_1665 (Interval in Earth days: 26) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.3 | 312. | -7.7 | 11.52 | 41.0 | 36.0 |
Layering in Lucus Planum: ESP_085895_1715 ESP_086330_1715 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.38 | 177. | -7.9 | 12.91 | 40.3 | 43.6 |
Diverse Materials in Western Jezero Crater Rim: ESP_085714_1985 ESP_085859_1985 (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 | 18.41 | 77.2 | -23. | -5.54 | 42.3 | 40.4 |
Pitted Ponded Crater with Glacial Lobe: ESP_085826_1425 ESP_085905_1425 (Interval in Earth days: 7) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.2 | 265. | -4.9 | 22.20 | 53.4 | 53.1 |
Giant Polygon Terminus: ESP_085849_2205 ESP_086996_2205 (Interval in Earth days: 90) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 39.92 | 346. | 2.02 | 17.45 | 50.4 | 42.0 |
Gullied Slope: ESP_085723_1370 ESP_085868_1370 (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 | -42.8 | 197. | -4.7 | 10.24 | 55.4 | 56.9 |
Candidate Future Landing Site in Horowitz Crater: ESP_085791_1480 ESP_086002_1480 (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 | -31.9 | 140. | -6.6 | -25.9 | 49.6 | 54.2 |
Inverted Channel in Noachis Terra: ESP_085941_1445 ESP_086231_1445 (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 | -35.0 | 4.25 | 0.71 | 12.20 | 53.5 | 57.5 |
Hillslope Morphologies near Holden Crater: ESP_085705_1550 ESP_085850_1550 (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 | -24.7 | 325. | 3.70 | 23.92 | 43.7 | 44.3 |
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