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.
| Candidate Landing Site for 2020 Mission in Gusev Crater: ESP_051845_1655 ESP_051911_1655 (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 | -14.5 | 175. | 14.2 | -7.79 | 52.3 | 54.3 |
| Lava-Draped Surface in Cerberus Palus: ESP_051991_1880 ESP_061156_1880 (Interval in Earth days: 714) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.848 | 147. | 2.70 | 26.28 | 42.1 | 43.4 |
| Pit in Upland among Troughs in Western Noctis Labyrinthus Region: ESP_051829_1755 ESP_063829_1755 (Interval in Earth days: 935) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.36 | 252. | -0.6 | 20.12 | 47.0 | 55.4 |
| Candidate Red Dragon Landing Site in Arcadia Planitia: ESP_051857_2210 ESP_051923_2210 (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 | 40.56 | 202. | -3.6 | -18.3 | 40.3 | 41.4 |
| Crater Filled with Ejecta: ESP_051787_1785 ESP_051286_1785 (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 | -1.65 | 317. | 11.1 | -17.1 | 44.3 | 41.4 |
| Lobate Features in Eastern Acidalia Planitia: ESP_051943_2270 ESP_052088_2270 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 46.83 | 12.9 | 0.98 | 12.26 | 41.8 | 40.4 |
| Sinuous Linear Gullies in Hellas Planitia: ESP_051836_1345 ESP_051770_1345 (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 | -45.3 | 67.2 | -4.7 | 11.68 | 75.7 | 74.0 |
| Outlet Breach in Small Crater: ESP_051967_1800 ESP_052112_1800 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.102 | 84.6 | -5.4 | 13.68 | 46.1 | 46.0 |
| Cracked Channel-Filling Deposit or Slumped Ejecta: ESP_051969_2095 ESP_052114_2095 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 29.20 | 25.8 | 1.30 | 16.21 | 37.9 | 36.8 |
| Sinuous Ridges and Valleys in Peridier Crater: ESP_051901_2055 ESP_052046_2055 (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 | 25.27 | 83.6 | -8.9 | 6.983 | 38.6 | 37.6 |
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