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.
| North-Pole-Facing Deposit in Crater Associated with Headwall Erosion: ESP_088186_2175 ESP_088753_2175 (Interval in Earth days: 45) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 37.39 | 260. | 0.31 | -14.6 | 42.8 | 45.7 |
| Dune Monitoring in North Mid-Latitude Crater: ESP_088311_2350 ESP_088377_2350 (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 | 54.61 | 83.4 | 5.81 | -7.40 | 45.0 | 46.2 |
| Dune Monitoring in North Mid-Latitude Crater: ESP_088261_2420 ESP_088182_2420 (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 | 61.94 | 6.66 | 6.67 | -7.68 | 47.4 | 48.6 |
| Sinuous Channel near Pavonis Mons: ESP_088358_1775 ESP_088569_1775 (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 | -2.36 | 248. | 13.3 | -2.87 | 56.0 | 57.4 |
| Channel South of Janssen Crater: ESP_088168_1800 ESP_088458_1800 (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 | 0.118 | 37.6 | -7.2 | 12.15 | 55.4 | 54.8 |
| Dune Field: ESP_088035_2385 ESP_088378_2385 (Interval in Earth days: 26) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 57.96 | 58.8 | 6.11 | -24.3 | 45.9 | 48.8 |
| Small Fresh Impact Crater: ESP_088159_1670 ESP_088726_1670 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.0 | 283. | 6.05 | -15.1 | 62.5 | 64.7 |
| Grooves and Undercutting in Columbia Valles: ESP_088171_1705 ESP_088316_1705 (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 | -9.60 | 316. | -5.9 | 3.691 | 61.1 | 60.9 |
| Obstacle within Lobate Debris Apron: ESP_088359_1435 ESP_088570_1435 (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 | -36.0 | 225. | 7.68 | -5.73 | 78.9 | 79.8 |
| Pits in North Polar Layered Deposits: ESP_088394_2650 ESP_088367_2650 (Interval in Earth days: 3) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 84.81 | 318. | -7.7 | 6.46 | 60.4 | 59.8 |
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