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.
| Central Pit Crater with Possibly Active Slope Processes: ESP_065704_1480 ESP_065770_1480 (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 | -31.6 | 191. | 7.68 | -6.72 | 46.3 | 46.6 |
| Fans and Polygons: ESP_065786_0925 ESP_065866_0925 (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 | -87.2 | 167. | 8.69 | 2.249 | 66.3 | 66.8 |
| Channel in Southern Highlands Crater: ESP_066064_1530 ESP_074281_1530 (Interval in Earth days: 640) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -26.6 | 87.9 | -7.6 | 2.974 | 43.6 | 48.8 |
| Landforms South of Isidis Planitia: ESP_066024_1820 ESP_075019_1820 (Interval in Earth days: 700) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 1.779 | 94.9 | 3.53 | -7.12 | 52.7 | 50.0 |
| Gully Monitoring and Topography: ESP_065837_1415 ESP_066589_1415 (Interval in Earth days: 59) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.0 | 163. | 4.75 | -23.9 | 45.1 | 41.7 |
| Outflow Channel from Morella Crater: ESP_065792_1700 ESP_057880_1700 (Interval in Earth days: 617) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.85 | 309. | -13. | 5.997 | 51.0 | 33.6 |
| Ridge in Eastern Candor Chasma: ESP_065819_1735 ESP_065885_1735 (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 | -6.66 | 291. | -3.2 | -17.7 | 51.2 | 51.6 |
| Channel Within Lava Flow Emanating from Aromatum Chaos: ESP_065818_1785 ESP_066227_1785 (Interval in Earth days: 31) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.49 | 317. | -2.7 | -25.8 | 53.4 | 51.1 |
| Raided Curvilinear Ridges: ESP_066022_1755 ESP_065956_1755 (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 | -4.63 | 151. | -7.5 | 6.58 | 50.4 | 50.1 |
| Cluster of Small Cones in Baetis Chaos: ESP_065977_1770 ESP_065911_1770 (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 | -2.86 | 299. | -7.7 | 6.708 | 51.7 | 51.3 |
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