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.
Canyon Walls in Coprates Chasma: ESP_087367_1655 ESP_087301_1655 (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 | -14.2 | 307. | 3.61 | 24.06 | 58.9 | 56.9 |
Layering within Yardangs: ESP_087477_1700 ESP_088334_1700 (Interval in Earth days: 67) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.71 | 184. | -2.1 | 18.83 | 57.3 | 60.0 |
North-Pole-Facing Deposit in Crater Associated with Headwall Erosion: ESP_087343_2220 ESP_087488_2220 (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 | 41.44 | 236. | -6.8 | 6.862 | 43.6 | 42.3 |
Irregular Cellular Structures around Crater in Arabia Terra: ESP_087496_2160 ESP_088630_2160 (Interval in Earth days: 88) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.47 | 20.2 | -7.3 | -22.0 | 42.9 | 46.2 |
Pitted Cone with Clear Moat: ESP_086926_2080 ESP_087071_2080 (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 | 27.85 | 102. | -8.9 | 4.814 | 42.3 | 41.3 |
Hillslope Morphologies near Murray Crater: ESP_087074_1555 ESP_087219_1555 (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 | -24.0 | 28.1 | -7.1 | 10.08 | 63.0 | 63.5 |
Small Shield Volcano East of Ascraeus Mons: ESP_087118_1920 ESP_087606_1920 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 11.96 | 261. | 5.03 | -20.6 | 43.8 | 48.5 |
Concentric Crater Fill: ESP_087124_2205 ESP_087190_2205 (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 | 40.20 | 93.4 | 5.73 | -9.98 | 42.7 | 43.9 |
Terrain in Chryse Planitia: ESP_087129_2145 ESP_087973_2145 (Interval in Earth days: 66) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 34.14 | 317. | 6.55 | -6.10 | 41.6 | 43.2 |
Small Mesa: ESP_087081_2175 ESP_087015_2175 (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 | 37.39 | 189. | -8.7 | 7.839 | 43.5 | 42.2 |
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