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.
| 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 |
| 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 |
| Fresh Impact Crater: ESP_084401_1440 ESP_085324_1440 (Interval in Earth days: 72) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -35.7 | 287. | 3.51 | -12.0 | 36.9 | 45.2 |
| North Branch of Kasei Valles East of Labeatis Mensa: ESP_084493_2060 ESP_084058_2060 (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 | 25.76 | 287. | 8.43 | -6.75 | 57.0 | 63.3 |
| Recent Crater: ESP_084414_1385 ESP_084770_1385 (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 | -41.2 | 293. | 7.28 | -8.40 | 38.5 | 41.5 |
| Landforms above Subsurface Radar Observations of South Polar Cap: ESP_084338_0965 ESP_084219_0965 (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 | -83.2 | 236. | -5.6 | 8.915 | 65.3 | 63.3 |
| Crater in Galaxias Fossae: ESP_084406_2175 ESP_093016_2175 (Interval in Earth days: 671) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.92 | 142. | -4.1 | 23.31 | 67.4 | 68.2 |
| 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 |
| Gully Monitoring: ESP_084450_1285 ESP_092335_1285 (Interval in Earth days: 615) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -50.9 | 33.5 | -7.5 | 4.851 | 44.2 | 46.0 |
| Dune Change Detection in Mawrth Vallis: ESP_084201_1980 ESP_084135_1980 (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 | 17.79 | 343. | -5.8 | 20.45 | 55.9 | 55.2 |
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