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.
| North-Central Endeavour Crater: ESP_019980_1780 ESP_018912_1780 (Interval in Earth days: 83) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.15 | 354. | 22.2 | -8.32 | 53.1 | 55.9 |
| The Beautiful Arc of a Dune: ESP_019992_1340 ESP_020269_1340 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -45.5 | 33.9 | 8.50 | -14.2 | 69.5 | 67.2 |
| Sinuous Ridges : ESP_019677_1585 ESP_019743_1585 (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 | -21.1 | 350. | 5.41 | -16.1 | 61.2 | 62.3 |
| Channel and Fan in Lyot Crater: ESP_019372_2300 ESP_024831_2300 (Interval in Earth days: 426) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 49.66 | 30.8 | -18. | -4.37 | 56.6 | 48.3 |
| Arc of Cones with Summit Pits in CTX Image: ESP_019577_1970 ESP_019867_1970 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 16.74 | 198. | -19. | 12.17 | 53.6 | 52.8 |
| Diverse Bedrock Exposures on Floor of Nili Patera: ESP_019595_1890 ESP_019740_1890 (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 | 9.085 | 67.0 | -15. | 1.288 | 53.9 | 53.1 |
| Exposure of North Polar Layered Deposits: ESP_019343_2685 ESP_028008_2685 (Interval in Earth days: 675) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 88.28 | 50.8 | -14. | -24.3 | 74.8 | 73.1 |
| Western Edge of Hellas Planitia: ESP_019596_1365 ESP_020084_1365 (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 | -43.2 | 44.5 | 8.05 | -14.8 | 73.1 | 68.8 |
| Barchan Dunes in Dulovo Crater Region: ESP_019357_1835 ESP_027216_1835 (Interval in Earth days: 613) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.672 | 84.6 | -7.6 | 7.029 | 53.8 | 51.2 |
| Rayed Crater in Arcadia Region in Themis V35985012: ESP_019590_2265 ESP_020078_2265 (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 | 46.31 | 197. | -0.0 | -17.7 | 56.8 | 65.6 |
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