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.
| Ice Deposition and Loss in an Impact Crater: ESP_032569_2225 ESP_033004_2225 (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 | 42.21 | 98.1 | -5.2 | 22.83 | 55.2 | 48.3 |
| Channel in the Cerberus Palus Region: ESP_032066_1860 ESP_040453_1860 (Interval in Earth days: 653) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 6.081 | 155. | 6.3 | -26.2 | 36.7 | 44.8 |
| Sediments in Ladon Basin: ESP_032297_1595 ESP_032719_1595 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -20.2 | 330. | 24.2 | 5.345 | 31.9 | 38.1 |
| Layers on Wall of Crater Interrupting Channel: ESP_031782_1990 ESP_031927_1990 (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 | 18.71 | 346. | 8.13 | 24.19 | 47.5 | 44.7 |
| USGS Dune Database 2308-691: ESP_031945_1105 ESP_032024_1105 (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 | -69.2 | 230. | 4.30 | 20.02 | 59.1 | 59.4 |
| Small Crater on South Polar Layered Deposits: ESP_031994_0920 ESP_032111_0920 (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 | -87.8 | 48.7 | 6.86 | 18.71 | 76.3 | 76.4 |
| Upland Valleys of Ladon Valles Basin: ESP_032073_1610 ESP_032007_1610 (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 | -18.9 | 326. | 9.50 | 26.89 | 31.5 | 29.8 |
| Exposure of South Polar Layered Deposits: ESP_031827_0940 ESP_031775_0940 (Interval in Earth days: 4) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -85.8 | 236. | 8.00 | -7.60 | 71.0 | 71.7 |
| Lava Draped Ridge on Western Margin of Echus Chasma: ESP_031890_1890 ESP_040145_1890 (Interval in Earth days: 643) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.936 | 281. | -16. | -0.76 | 41.4 | 48.5 |
| Crater in Elysium Planitia: ESP_031842_1865 ESP_084775_1865 (Interval in Earth days: 4125) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 6.615 | 150. | 2.46 | -7.69 | 39.4 | 42.1 |
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