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.
| Line of Cones and Associated Flows in Arsia Sulci: PSP_007603_1770 ESP_036718_1770 (Interval in Earth days: 2269) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.83 | 231. | 8.18 | -17.6 | 47.1 | 57.8 |
| Russell Crater Dunes: PSP_007018_1255 PSP_007229_1255 (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 | -54.2 | 12.9 | 3.27 | -5.25 | 73.2 | 77.0 |
| Streamlined Form North of Mangala Valles: PSP_007683_1805 PSP_009542_1805 (Interval in Earth days: 145) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.500 | 207. | -3.0 | -16.3 | 47.1 | 56.6 |
| Gullies: PSP_007031_2220 PSP_009826_2220 (Interval in Earth days: 218) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 41.43 | 4.84 | 2.91 | 18.33 | 45.6 | 45.0 |
| Wrinkle Ridge: PSP_007052_1870 ESP_016361_1870 (Interval in Earth days: 726) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.101 | 156. | -6.0 | 26.66 | 39.8 | 40.6 |
| Fresh 7-Kilometer Diameter Crater with Bright Rayed Ejecta: PSP_007731_2060 ESP_026310_2060 (Interval in Earth days: 1448) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 25.77 | 333. | 1.95 | 28.52 | 40.6 | 38.7 |
| Dune Field in Impact Crater Near Cerberus Fossae: PSP_008159_1885 PSP_008449_1885 (Interval in Earth days: 22) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.564 | 169. | -6.9 | 2.406 | 47.4 | 48.2 |
| Polygonal Fractures in Utopia Planitia: PSP_008069_2195 PSP_008504_2195 (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 | 38.95 | 102. | -5.9 | 5.466 | 42.2 | 41.3 |
| Well-Exposed Central Uplift in Unnamed Crater: PSP_007252_1615 ESP_015981_1615 (Interval in Earth days: 680) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -18.4 | 98.7 | -0.9 | -22.0 | 52.1 | 52.3 |
| Deposits in Kasei Valles: PSP_007970_2015 ESP_033551_2015 (Interval in Earth days: 1993) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.06 | 287. | -0.6 | 17.86 | 42.0 | 36.8 |
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