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.
| Thin Layers in Eroded Crater Southwest of Bamberg Crater : ESP_046142_2165 ESP_046643_2165 (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 | 36.34 | 355. | -6.1 | 12.42 | 52.7 | 58.2 |
| Valleys and Fractures on Alba Mons : ESP_045869_2270 ESP_046304_2270 (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 | 46.52 | 246. | -2.9 | 22.47 | 52.0 | 56.5 |
| Light-Toned Surface in Valley in CTX Image : ESP_046011_1620 ESP_046723_1620 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -17.8 | 338. | -6.0 | 11.19 | 57.7 | 52.7 |
| High-Latitude Exposure of North Polar Layered Deposits : ESP_045943_2685 ESP_045454_2685 (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 | 88.57 | 34.3 | -27. | -21.8 | 78.0 | 70.7 |
| Layered-Target Crater : ESP_045847_2290 ESP_051042_2290 (Interval in Earth days: 405) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 48.57 | 127. | -3.9 | 23.69 | 52.6 | 47.2 |
| Possible Sulfate and Clay Mixture with Alunite : ESP_046148_1540 ESP_064174_1540 (Interval in Earth days: 1404) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -25.6 | 198. | 4.34 | -11.3 | 59.9 | 62.8 |
| Channel in Maadim Vallis : ESP_045951_1560 ESP_046162_1560 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -23.5 | 176. | 7.72 | -1.89 | 60.0 | 59.2 |
| Stratigraphy of Crater Floor Materials : ESP_046035_1595 ESP_045969_1595 (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 | -20.4 | 42.6 | 7.58 | 28.87 | 57.9 | 56.7 |
| Light-Toned Deposits in Western Gorgonum Chaos : ESP_045977_1405 ESP_060469_1405 (Interval in Earth days: 1129) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.9 | 190. | -10. | 0.139 | 69.8 | 68.6 |
| Pasithea Dorsum : ESP_045801_1240 ESP_045867_1240 (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 | -55.5 | 317. | 2.41 | -12.1 | 81.7 | 81.9 |
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