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.
A Slice through the Layercake: ESP_084979_1975 ESP_085045_1975 (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 | 17.49 | 336. | 16.6 | -4.34 | 44.6 | 45.3 |
North Pole Facing Deposit in Crater: ESP_085774_2230 ESP_085853_2230 (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 | 42.65 | 234. | 0.49 | 23.69 | 53.0 | 50.5 |
Avalanches on Walls of Gully in Echus Fossae: ESP_085957_1810 ESP_086880_1810 (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 | 1.056 | 282. | 3.62 | -19.7 | 38.1 | 47.9 |
Exposure of Layered Materials along Hellas Planitia Rim Escarpment: ESP_085807_1590 ESP_086242_1590 (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 | -20.7 | 63.1 | -16. | 0.443 | 44.6 | 49.5 |
Raised Circular Feature: ESP_085811_2210 ESP_086246_2210 (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 | 40.81 | 305. | -6.0 | 6.055 | 51.8 | 47.1 |
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 |
Kasei Valles Lava: ESP_085970_1965 ESP_086326_1965 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 16.39 | 285. | 4.76 | -6.69 | 38.9 | 40.3 |
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 |
Kasei Valles Lava: ESP_085825_1965 ESP_085614_1965 (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 | 16.14 | 285. | 4.28 | -6.99 | 39.1 | 40.5 |
Hillslope Morphologies in Crater: ESP_085793_1510 ESP_086294_1510 (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 | -28.6 | 84.7 | 3.79 | -4.91 | 47.1 | 55.3 |
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