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.
| South Facing Gullies with Inverted Aprons: ESP_084300_1410 ESP_084234_1410 (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 | -38.8 | 166. | -3.6 | 19.20 | 38.3 | 36.7 |
| Streamline Feature Surrounding Crater in Ares Vallis: ESP_084162_1985 ESP_084373_1985 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.12 | 327. | -2.4 | -21.9 | 56.4 | 55.0 |
| Central Russell Crater Erg: ESP_084253_1250 ESP_084464_1250 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -54.4 | 12.6 | -1.5 | -12.1 | 44.9 | 46.6 |
| Landforms above Subsurface Radar Observations of South Polar Cap: ESP_084325_1000 ESP_084562_1000 (Interval in Earth days: 19) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -80.0 | 222. | -6.3 | 13.65 | 62.6 | 64.0 |
| Inverted Channel in Noachis Terra: ESP_084385_1585 ESP_084451_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 | 2.82 | 0.76 | -22.6 | 35.6 | 37.2 |
| Possible Well-Exposed Overturned Terrain in Crater near Her Desher Vallis: ESP_084321_1550 ESP_084400_1550 (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 | -24.7 | 311. | -7.1 | 25.15 | 36.4 | 33.4 |
| Well-Preserved Impact Crater: ESP_084209_1585 ESP_084644_1585 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -21.0 | 128. | 4.91 | 22.15 | 36.6 | 32.9 |
| Possible Volcanic Edifice in Terra Sirenum: ESP_084206_1530 ESP_084562_1530 (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 | -26.8 | 211. | 2.15 | -8.24 | 36.4 | 35.9 |
| Resistant Material in Olympus Mons Aureole Ridges: ESP_084192_2110 ESP_075502_2110 (Interval in Earth days: 677) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 30.57 | 226. | 3.71 | -6.18 | 64.8 | 63.6 |
| Fresh 500-meter Diameter Impact Crater: ESP_084408_1745 ESP_085199_1745 (Interval in Earth days: 62) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.54 | 93.1 | -3.5 | 19.38 | 39.7 | 33.7 |
Page 89 of 913 (9,124 images) | |||||