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.
| Gullies Monitoring near Ogygis Undae: ESP_066083_1295 ESP_066571_1295 (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 | -50.2 | 292. | 3.28 | 17.14 | 45.3 | 42.7 |
| Ares Vallis: ESP_065791_1920 ESP_066200_1920 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 11.67 | 333. | -3.6 | -25.0 | 60.4 | 58.6 |
| Landforms South of Isidis Planitia: ESP_066024_1820 ESP_075019_1820 (Interval in Earth days: 700) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 1.779 | 94.9 | 3.53 | -7.12 | 52.7 | 50.0 |
| Debris Flows on Eos Chasma Walls: ESP_065950_1665 ESP_065884_1665 (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 | -13.3 | 317. | -8.6 | 5.799 | 47.8 | 47.5 |
| Aram Chaos: ESP_066015_1815 ESP_065804_1815 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 1.686 | 339. | 12.8 | -7.98 | 52.1 | 55.4 |
| Layering in Western Arabia Terra: ESP_065909_1895 ESP_065975_1895 (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 | 9.623 | 352. | 6.43 | -7.49 | 57.8 | 58.2 |
| Slope Failures in Tempe Terra: ESP_065925_2175 ESP_066057_2175 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 37.31 | 273. | -9.9 | -28.1 | 76.5 | 77.1 |
| Active Gully in Matara Crater: ESP_065789_1300 ESP_065934_1300 (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 | -49.4 | 34.8 | 7.58 | 29.10 | 47.6 | 44.3 |
| Mesa in Low Northern Latitudes: ESP_066046_1900 ESP_073973_1900 (Interval in Earth days: 618) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.890 | 213. | 2.52 | -8.89 | 57.1 | 61.0 |
| Raided Curvilinear Ridges: ESP_066022_1755 ESP_065956_1755 (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 | -4.63 | 151. | -7.5 | 6.58 | 50.4 | 50.1 |
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