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.
| Loose Cluster of Zunil Crater Secondary Craters: PSP_003874_1815 PSP_004375_1815 (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 | 1.259 | 162. | 4.39 | 27.49 | 53.1 | 47.0 |
| Low Shield with Radial Flows East of the Olympica Fossae: PSP_003818_2040 PSP_004108_2040 (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 | 23.71 | 249. | -3.0 | 23.54 | 66.1 | 63.7 |
| Mounds in Utopia Region: PSP_004180_2165 ESP_012434_2165 (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 | 36.22 | 83.9 | 4.54 | 18.73 | 73.4 | 72.7 |
| Light-Toned Layering in Plains South of Ius Region: PSP_003382_1715 PSP_004371_1715 (Interval in Earth days: 78) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.67 | 276. | 7.75 | -2.93 | 52.5 | 44.4 |
| Boulders on Lobate Ejecta: PSP_003484_1305 PSP_003563_1305 (Interval in Earth days: 7) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -49.3 | 18.5 | -7.9 | 19.01 | 55.3 | 52.1 |
| Gullies in the Wall of a Large Pit in Southern Noachia: PSP_003287_1115 PSP_003511_1115 (Interval in Earth days: 18) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -68.3 | 1.15 | -2.0 | 20.02 | 66.2 | 60.9 |
| Possible Granitoid Unit in Syrtis Major: PSP_003205_2000 PSP_003706_2000 (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 | 19.92 | 65.8 | -8.5 | 17.38 | 62.9 | 62.5 |
| Phyllosilicate-Rich Area: PSP_004329_2045 ESP_013282_2045 (Interval in Earth days: 698) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.37 | 338. | -2.8 | -25.9 | 64.5 | 65.4 |
| Dike and/or Fault Splay in the Coloe Fossae Region: PSP_004181_2170 ESP_021560_2170 (Interval in Earth days: 1354) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.57 | 56.7 | 3.06 | -15.9 | 73.7 | 74.5 |
| The Ponded and Pitted Floor of Hale Crater : PSP_004132_1435 ESP_012742_1435 (Interval in Earth days: 671) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -36.0 | 324 | 2.63 | 22.65 | 42.2 | 44.5 |
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