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.
| Thick CO2 Ice Mesas: ESP_068208_0955 ESP_084604_0845 (Interval in Earth days: 1277) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -84.4 | 291. | 9.83 | -8.68 | 88.8 | 76.7 |
| Layers Exposed in Margins of Two Fans or Deltas: ESP_068189_2015 ESP_069047_2015 (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 | 21.48 | 57.8 | 14.9 | -4.57 | 44.1 | 47.0 |
| Parallel Ridges on Northeast Floor of Barnard Crater: ESP_068110_1190 ESP_076669_1190 (Interval in Earth days: 667) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -60.5 | 62.4 | 23.5 | -5.24 | 68.6 | 64.2 |
| Expanded Secondary Crater Cluster in Arcadia Planitia: ESP_068250_2220 ESP_069187_2220 (Interval in Earth days: 73) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 41.65 | 193. | -8.2 | 0.857 | 54.4 | 49.0 |
| Crater Ejecta in Tyrrhena Terra: ESP_068453_1775 ESP_069812_1775 (Interval in Earth days: 106) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.27 | 61.4 | 5.89 | -5.19 | 44.7 | 59.1 |
| Eos Chasma Slumps: ESP_068444_1630 ESP_067718_1630 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -16.6 | 310. | -18. | 14.65 | 51.0 | 39.5 |
| Jezero Crater Inlet Valley: ESP_068228_1990 ESP_072000_1990 (Interval in Earth days: 294) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.61 | 76.5 | -7.0 | 14.20 | 44.9 | 49.9 |
| Crater with Outlet Channel in Southern Highlands: ESP_068258_1480 ESP_073665_1480 (Interval in Earth days: 421) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -31.5 | 344. | -6.6 | 9.163 | 54.4 | 56.4 |
| Nepenthes Mensae: ESP_067738_1885 ESP_085343_1885 (Interval in Earth days: 1372) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.355 | 122. | 1.93 | -8.16 | 41.8 | 38.9 |
| Complex Crater Fill and Erosion: ESP_067822_1860 ESP_067690_1860 (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 | 6.047 | 352. | -8.4 | 7.125 | 42.0 | 40.8 |
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