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-Related Pitted Materials in 10-Kilometer Crater near Amazonis Planitia : ESP_092316_1890 ESP_092817_1890 (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 | 8.990 | 184. | 3.46 | -21.4 | 56.4 | 53.0 |
| Thermal Anomaly in Young Lava Flows of Elysium Mons: ESP_092633_1960 ESP_092989_1960 (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 | 15.59 | 165. | 13.9 | 2.663 | 57.1 | 53.8 |
| Channel within Valley in Margaritifer Terra: ESP_092587_1705 ESP_092798_1705 (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 | -9.47 | 345. | 3.42 | -20.4 | 44.3 | 43.5 |
| South Polar Glacier Crevasses: ESP_092682_0915 ESP_092589_0915 (Interval in Earth days: 8) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -88.6 | 323. | 22.6 | 26.11 | 64.9 | 64.3 |
| Banded or Layered Megabreccia Clasts in Nili Fossae: ESP_092544_1995 ESP_092610_1995 (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 | 19.17 | 76.5 | -1.1 | -26.7 | 61.3 | 62.3 |
| Rock Glacier-Like Feature: ESP_092547_1380 ESP_092758_1380 (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 | -41.5 | 1.56 | 8.51 | -12.4 | 40.9 | 40.6 |
| Dune Field: ESP_092590_1725 ESP_092946_1725 (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 | -7.35 | 263. | -4.9 | -19.7 | 45.7 | 42.6 |
| Landforms above Subsurface Radar Observations of South Polar Cap: ESP_092561_0990 ESP_084729_0990 (Interval in Earth days: 610) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -81.0 | 352. | 10.6 | -5.34 | 60.0 | 68.1 |
| Possible Pit in USGS Cave Candidate Catalog Entry Number CC0518: ESP_092445_1920 ESP_093157_1920 (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 | 11.84 | 260. | 4.97 | -20.1 | 57.0 | 50.5 |
| Possible Undercutting along Streamline Feature in Elaver Vallis: ESP_091995_1705 ESP_092272_1705 (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 | -9.35 | 309. | 4.49 | -12.4 | 50.6 | 49.1 |
Page 11 of 896 (8,955 images) | |||||