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.
| Highland Channels: ESP_073604_1340 ESP_064780_1340 (Interval in Earth days: 687) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -45.8 | 215. | -23. | 7.346 | 63.4 | 61.2 |
| Layered Rock in Hollow on Mesa-Top: ESP_073607_1825 ESP_073673_1825 (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 | 2.246 | 123. | 8.32 | -12.3 | 57.3 | 58.9 |
| Intersection of Aeolis Serpens with Crater Rim: ESP_073870_1820 ESP_073527_1820 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.154 | 147. | -26. | 8.608 | 60.0 | 57.3 |
| Cyclic Stratigraphy of Kaporo Crater Mound: ESP_073677_1800 ESP_073822_1800 (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 | -0.11 | 14.5 | -7.3 | 15.98 | 58.1 | 56.0 |
| Chaotic Terrain in Xanthe Terra: ESP_073666_1780 ESP_074154_1780 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.08 | 315. | -8.4 | -28.3 | 57.8 | 57.6 |
| Small Delta or Fan: ESP_073635_1505 ESP_073912_1505 (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 | -29.3 | 84.5 | -4.5 | -18.3 | 57.4 | 55.2 |
| Bright Linear Dunes West of Meroe Patera: ESP_073886_1875 ESP_074242_1875 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.658 | 67.5 | 4.76 | 14.34 | 59.2 | 57.8 |
| Deposits in Ganges Chasma: ESP_073732_1715 ESP_066491_1715 (Interval in Earth days: 564) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.58 | 311. | 19.7 | -7.10 | 54.3 | 43.8 |
| Small Delta or Fan: ESP_073767_1475 ESP_074255_1475 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -32.0 | 81.4 | -1.4 | -25.8 | 56.0 | 51.5 |
| Fresh Cratering Covering Crater Rim: ESP_073752_1715 ESP_072908_1715 (Interval in Earth days: 66) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.33 | 129. | -22. | -7.76 | 57.6 | 59.0 |
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