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.
Well-Exposed Scarp of Noachian Phyllosilicates Along Nili Fossae: PSP_007200_2005 ESP_016153_2005 (Interval in Earth days: 698) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 20.03 | 73.6 | 1.53 | 26.79 | 39.1 | 37.1 |
Mojave Crater Southern Rim - Putative Melt-Bearing Flows: PSP_007995_1875 PSP_009432_1875 (Interval in Earth days: 112) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.168 | 327. | -3.2 | 15.34 | 46.7 | 50.9 |
Vertical Exposure of Layering in West Candor Chasma: PSP_007021_1740 PSP_007232_1740 (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 | -5.82 | 283. | 5.28 | -9.86 | 42.3 | 45.8 |
Bright Gully Fans: PSP_007429_2440 PSP_008141_2440 (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 | 63.78 | 292. | 2.14 | -7.16 | 55.0 | 50.5 |
Crater with Gullies: PSP_007652_2230 ESP_024095_2230 (Interval in Earth days: 1282) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 42.65 | 328. | -6.0 | -27.7 | 43.8 | 52.7 |
3-Kilometer Diameter Crater with Good Bedrock Exposures in Upper Walls: PSP_007892_1865 ESP_079800_1865 (Interval in Earth days: 5603) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 6.625 | 259. | 4.25 | -7.35 | 45.6 | 54.0 |
Faults in Ius Chasma: PSP_008010_1720 PSP_009658_1720 (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 | -7.82 | 279. | -4.9 | 7.572 | 54.5 | 59.5 |
Granicus Valles Subchannel Breakout From Main Channel: PSP_007725_2075 PSP_007936_2075 (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 | 27.11 | 136. | 7.86 | -8.35 | 40.0 | 41.8 |
Chasma Borealis: PSP_007020_2580 PSP_007178_2580 (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 | 77.78 | 292. | 0 | 12.81 | 69.8 | 67.1 |
Hellas Planitia: PSP_007715_1420 ESP_016022_1420 (Interval in Earth days: 647) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.4 | 57.6 | 8.36 | 23.98 | 70.4 | 62.4 |
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