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.
| Crater in Arabia Terra: ESP_079664_2185 ESP_079519_2185 (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 | 38.16 | 6.10 | 7.88 | -6.68 | 43.8 | 44.6 |
| Dune Monitoring in Northern Mid-Latitude Crater: ESP_079424_2385 ESP_087916_2385 (Interval in Earth days: 661) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 58.24 | 74.8 | 0.41 | -29.1 | 47.0 | 49.3 |
| Barchan Dunes in North Polar Layered Deposits: ESP_079724_2645 ESP_080053_2645 (Interval in Earth days: 26) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 84.33 | 137. | 2.16 | 16.70 | 59.9 | 60.7 |
| Possible Vent Region within Volcanic Plains: ESP_079677_1830 ESP_080033_1830 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.796 | 17.0 | -3.4 | 19.86 | 55.4 | 54.3 |
| Small Icy Scarp: ESP_079484_2305 ESP_079207_2305 (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 | 50.17 | 241. | -16. | -1.78 | 46.4 | 44.9 |
| Ridged Flow-Like Features in Deuteronilus Mensae: ESP_079650_2225 ESP_079795_2225 (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 | 42.01 | 27.6 | 7.83 | 20.95 | 43.7 | 43.0 |
| Scarp Monitoring: ESP_079498_2345 ESP_079419_2345 (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 | 54.19 | 214. | 7.16 | -13.8 | 45.3 | 47.1 |
| West Olympia Region Polar Aeolian-Ice Landforms: ESP_079779_2600 ESP_079660_2600 (Interval in Earth days: 9) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 79.77 | 91.2 | 0.43 | 15.04 | 57.3 | 56.2 |
| Pit in Hephaestus Fossae: ESP_079739_2015 ESP_080227_2015 (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 | 21.50 | 122. | -4.8 | -16.8 | 47.8 | 50.4 |
| Wall of Orson Welles Crater: ESP_079798_1785 ESP_080075_1785 (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 | -1.52 | 313. | 2.76 | -14.8 | 57.6 | 59.1 |
Page 96 of 878 (8,771 images) | |||||