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.
| Well-Preserved 4-Kilometer Impact Crater: ESP_083095_1535 ESP_083240_1535 (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 | -26.2 | 307. | -5.3 | 9.499 | 49.9 | 46.9 |
| Fresh Crater near Ice-Rich Terrain: ESP_083188_1295 ESP_083254_1295 (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 | -50.3 | 290. | 7.09 | -8.45 | 50.5 | 50.7 |
| Channel Edge with Overbank Flow Deposits: ESP_083033_1835 ESP_082967_1835 (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 | 3.456 | 195. | 7.43 | 29.20 | 57.0 | 55.5 |
| Eroded Landform in Chryse Planitia: ESP_083121_1940 ESP_083767_1940 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 13.87 | 312. | -4.9 | 22.98 | 62.5 | 56.4 |
| Flow Features on Ice-Rich Plateau on Malea Patera: ESP_083276_1165 ESP_083144_1165 (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 | -63.1 | 53.5 | -7.0 | 15.29 | 55.0 | 55.2 |
| Channel Entering Crater: ESP_082956_1395 ESP_083378_1395 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -40.3 | 143. | 4.73 | -7.28 | 51.9 | 46.6 |
| Pitted Material: ESP_083282_1425 ESP_083928_1425 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.2 | 242. | 4.8 | 21.65 | 46.8 | 37.9 |
| Ariadnes Colles: ESP_083100_1450 ESP_083588_1450 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -34.6 | 171. | 3.68 | -22.4 | 49.2 | 44.5 |
| Planned ExoMars Landing Site in Oxia Planum: ESP_083041_1980 ESP_082975_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 | 17.80 | 335. | 2.09 | 23.42 | 64.3 | 62.7 |
| Channel in Valley near Tyrrhena Patera: ESP_083076_1590 ESP_083142_1590 (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 | -20.6 | 104. | 3.93 | -19.6 | 50.0 | 51.0 |
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