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.
| Light-Toned Rocks inside a Crater: ESP_017292_1680 ESP_025375_1680 (Interval in Earth days: 630) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.8 | 304. | -4.3 | 26.62 | 59.6 | 50.6 |
| Pits along Fractures in Crater Floor Material: ESP_017103_2255 ESP_018092_2255 (Interval in Earth days: 77) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 44.98 | 57.3 | -5.1 | -18.6 | 42.6 | 44.8 |
| Viscous Flow in Protonilus Mensae: ESP_017024_2230 ESP_017314_2230 (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 | 42.61 | 55.3 | -10. | 8.248 | 42.7 | 40.9 |
| Nili Patera: ESP_016905_1890 ESP_035181_1890 (Interval in Earth days: 1424) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.910 | 67.6 | 0 | 17.66 | 45.7 | 47.4 |
| Persbo Crater Ejecta Covered by Lava Flows: ESP_017060_1890 ESP_017205_1890 (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 | 8.912 | 156. | -8.7 | 5.039 | 47.2 | 46.8 |
| Fans in Unnamed Crater Southeast of Holden Crater: ESP_017278_1470 ESP_053725_1470 (Interval in Earth days: 2840) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -32.4 | 329. | -2.9 | 7.278 | 73.9 | 72.6 |
| Central Structure and Layered Bedrock in 25-Kilometer Diameter Crater: ESP_017002_1535 ESP_017147_1535 (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 | -26.0 | 303. | -3.1 | 10.15 | 67.4 | 67.7 |
| Light-Toned Mounds in Acidalia Planitia: ESP_017132_2250 ESP_017633_2250 (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 | 44.43 | 345. | -6.6 | 5.659 | 42.7 | 41.6 |
| Exposure of Lower Layers in South Melas Chasma with Stratigraphic Contacts: ESP_016963_1680 ESP_018598_1680 (Interval in Earth days: 127) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.1 | 286. | -0.9 | 16.30 | 57.5 | 60.1 |
| Enigmatic Pits in Southern Elysium Planitia: ESP_017284_1790 ESP_017429_1790 (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 | -1.07 | 160. | 5.24 | 19.21 | 52.3 | 52.0 |
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