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.
| Going with the Flow: ESP_075639_1420 ESP_076140_1420 (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 | -37.7 | 95.5 | -6.3 | 8.269 | 38.2 | 40.4 |
| An Inlet Channel to Jezero Crater : ESP_076523_1990 ESP_076180_1990 (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 | 18.65 | 76.6 | -20. | 6.667 | 44.4 | 45.8 |
| Ancient Fluvial Activity: ESP_076507_1735 ESP_075808_1735 (Interval in Earth days: 54) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.38 | 153. | 9.25 | 27.49 | 34.8 | 34.9 |
| Two-Color Aeolian Ridges: ESP_076582_1730 ESP_076925_1730 (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 | -6.92 | 267. | 0 | -15.5 | 35.8 | 39.4 |
| Small Delta or Fan: ESP_076604_2150 ESP_077290_2150 (Interval in Earth days: 53) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 34.90 | 21.3 | 4.73 | -10.0 | 51.7 | 46.6 |
| Layering in Western Arabia Terra: ESP_076447_1900 ESP_075959_1900 (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 | 9.843 | 351. | -19. | -5.22 | 40.8 | 43.7 |
| Dark Layers in Arabia Crater: ESP_076460_1910 ESP_076671_1910 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 10.61 | 355. | -2.3 | 9.977 | 39.8 | 37.9 |
| Youthful Crater in THEMIS V22898007 and at Edge of MOC E11-03928: ESP_076415_1345 ESP_084037_1345 (Interval in Earth days: 594) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -45.2 | 150. | 5.97 | -6.29 | 48.5 | 41.2 |
| Crater in Arabia Terra: ESP_076631_2175 ESP_077462_2175 (Interval in Earth days: 65) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 37.29 | 5.51 | -8.7 | 7.098 | 53.9 | 45.4 |
| Channel in Nereidum Montes: ESP_076488_1440 ESP_076831_1440 (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 | -35.4 | 316. | 7.92 | -8.22 | 43.5 | 49.7 |
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