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.
| Exposure of South Polar Layered Deposits: ESP_031954_0925 ESP_032137_0925 (Interval in Earth days: 14) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.3 | 62.5 | -0.0 | 14.03 | 75.9 | 76.8 |
| Richardson Crater Dunes Summer Monitoring: ESP_031881_1080 ESP_031749_1080 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -72.0 | 179. | 2.32 | 16.78 | 60.4 | 57.9 |
| Floor of East Candor Chasma: ESP_031916_1730 ESP_031982_1730 (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 | -6.84 | 292. | -6.5 | -25.3 | 33.7 | 35.0 |
| Exposure of South Polar Layered Deposits: ESP_031777_0915 ESP_031937_0915 (Interval in Earth days: 13) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -88.3 | 172. | 20.9 | 14.91 | 71.8 | 75.4 |
| Athabasca Valles Source Region: ESP_031789_1900 ESP_047336_1900 (Interval in Earth days: 1211) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.950 | 157. | -3.9 | 27.30 | 42.3 | 52.8 |
| 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 |
| Portion of Mound in Gale Crater: ESP_031803_1750 ESP_031948_1750 (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 | -4.99 | 137. | -13. | 6.521 | 35.5 | 33.1 |
| Hourglass Channel Network in Aeolis Planum: ESP_031908_1740 ESP_040440_1740 (Interval in Earth days: 665) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.98 | 149. | 10.1 | -2.24 | 32.7 | 37.4 |
| Search for Clinoforms in Delta Candidate: ESP_031921_1750 ESP_039820_1750 (Interval in Earth days: 616) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.93 | 155. | -4.9 | 6.516 | 34.1 | 44.3 |
| 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 |
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