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.
| Possible Fossil Dunes in Noachis Terra: ESP_032941_1310 ESP_033020_1310 (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 | -48.9 | 34.0 | -2.6 | 22.11 | 60.1 | 60.2 |
| Impact Crater with Central Peak: ESP_033202_1685 ESP_060393_1685 (Interval in Earth days: 2119) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.5 | 101. | 2.77 | -6.13 | 40.8 | 49.3 |
| Dark Sediments in the Medusae Fossae Formation: ESP_032910_1795 ESP_033411_1795 (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 | -0.53 | 153. | -6.3 | 6.617 | 35.6 | 38.9 |
| Pedestal Crater in Arcadia Planitia: ESP_032921_2355 ESP_033145_2355 (Interval in Earth days: 18) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 55.13 | 204. | -0.0 | 22.74 | 59.9 | 55.7 |
| Complex of Fresh Shallow Valleys: ESP_033134_1385 ESP_068014_1385 (Interval in Earth days: 2718) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -41.3 | 162. | -0.6 | -21.4 | 57.7 | 56.8 |
| Western Portion of Possible Multiple Impact in Arabia Terra: ESP_033272_1840 ESP_033417_1840 (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 | 4.045 | 349. | -3.5 | 10.60 | 37.5 | 37.5 |
| Large Meander in Sinuous Ridge in Aeolis Region: ESP_033187_1780 ESP_034321_1780 (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 | -1.77 | 150. | -1.5 | 7.93 | 37.7 | 48.4 |
| Possible Preserved Impact Melt Flow on the Ejecta of Bakhuysen Crater: ESP_033258_1555 ESP_033469_1555 (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 | -24.1 | 14.1 | 6.09 | -3.25 | 47.9 | 51.7 |
| Possible Terraced Crater in Arcadia Planitia: ESP_033066_2230 ESP_033501_2230 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 42.78 | 209. | -7.0 | 19.40 | 50.0 | 44.4 |
| Massif in Northwest Hellas Region: ESP_033006_1545 ESP_033296_1545 (Interval in Earth days: 22) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -25.0 | 55.1 | 2.01 | 24.62 | 44.9 | 47.9 |
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