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.
| Western Rim and Ejecta of Well-Preserved Impact Crater : ESP_059458_1610 ESP_059392_1610 (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 | -18.6 | 68.9 | -14. | 7.85 | 41.0 | 38.5 |
| Lava Flows Embaying Impact Crater: ESP_059452_1540 ESP_076135_1540 (Interval in Earth days: 1300) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -25.9 | 232. | -0.5 | -15.5 | 44.0 | 37.4 |
| Dense Network of Ridges and Alcoves along Crater Rim : ESP_059460_1820 ESP_059605_1820 (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 | 2.028 | 11.1 | -6.9 | 10.19 | 34.2 | 33.8 |
| Well-Preserved Small Impact Crater on Hellas Planitia Floor : ESP_059261_1380 ESP_067886_1380 (Interval in Earth days: 672) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -41.7 | 49.7 | -4.4 | 21.24 | 51.7 | 52.2 |
| Weathered Ejecta and Pitted Material Associated with Kontum Crater : ESP_059397_1480 ESP_051076_1480 (Interval in Earth days: 648) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -31.8 | 293. | 17.9 | 1.328 | 45.8 | 54.7 |
| Possible Olivine-Rich Crater in Terra Sirenum : ESP_059322_1515 ESP_076783_1515 (Interval in Earth days: 1361) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -28.2 | 182. | -5.0 | 23.12 | 43.6 | 42.7 |
| Gullied Lobate Flow Features : ESP_059436_1335 ESP_059001_1335 (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 | -46.3 | 310. | 14.6 | -19.1 | 57.1 | 51.5 |
| Ancient Bedforms on Gordii Dorsum : ESP_059268_1895 ESP_059545_1895 (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 | 9.495 | 210. | 6.39 | -21.1 | 33.0 | 35.9 |
| Impact Crater with Central Pit : ESP_059263_1840 ESP_059408_1840 (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 | 4.060 | 349. | -8.6 | 7.628 | 33.4 | 32.6 |
| Terminus of Pitted Materials Emanating from Oudemans Crater : ESP_059411_1735 ESP_059266_1735 (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 | -6.34 | 269. | 2.11 | -14.5 | 34.4 | 34.3 |
Page 274 of 896 (8,955 images) | |||||