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.
| Terraced Impact Crater on Lobate Debris Apron: ESP_084759_1385 ESP_084825_1385 (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 | -40.9 | 232. | 2.14 | -19.6 | 40.6 | 42.6 |
| Ancient Crust Outcrops at Nectaris Montes: ESP_084519_1650 ESP_084018_1650 (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 | -14.7 | 304. | -17. | -6.83 | 37.1 | 40.8 |
| Southeast Aeolis Dorsa Inverted Delta Trunk Channel: ESP_084854_1735 ESP_084999_1735 (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 | -6.32 | 154. | -2.4 | 9.423 | 36.0 | 34.5 |
| Streamlined Features in Granicus Valles: ESP_084815_2075 ESP_085936_2075 (Interval in Earth days: 87) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 27.48 | 133. | 7.85 | -9.82 | 54.0 | 43.9 |
| Landforms above Subsurface Radar Observations of South Polar Cap: ESP_084674_0970 ESP_084648_0970 (Interval in Earth days: 2) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -82.8 | 55.2 | 1.85 | -13.0 | 68.4 | 69.1 |
| Landforms above Subsurface Radar Observations of South Polar Cap: ESP_084894_1050 ESP_084762_1050 (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 | -75.0 | 156. | -0.7 | 14.00 | 65.3 | 62.6 |
| Streamlined Features in Hebrus Valles: ESP_084868_1995 ESP_085567_1995 (Interval in Earth days: 54) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 19.18 | 127. | 9.06 | -7.83 | 47.5 | 42.1 |
| Potential Fan Deposit at Head of Mawrth Vallis: ESP_084715_1990 ESP_085005_1990 (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 | 18.91 | 346. | -0.5 | 15.83 | 49.8 | 45.3 |
| Overlapping Debris Aprons within Ganges Chasma: ESP_084848_1720 ESP_085138_1720 (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 | -8.01 | 318. | -8.1 | 20.34 | 36.1 | 33.3 |
| Terminus of Fissure in Athabasca Valles: ESP_084867_1900 ESP_085078_1900 (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 | 9.761 | 156. | 0.88 | -9.17 | 42.3 | 41.1 |
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