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.
| Circular Features in Western Elysium Planitia: ESP_020911_1850 ESP_021623_1850 (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 | 4.702 | 138. | -7.0 | 3.973 | 56.5 | 53.1 |
| Ridges in Meridiani Planum: ESP_020573_1805 ESP_021562_1805 (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 | 0.248 | 6.10 | 3.45 | -11.8 | 54.8 | 52.5 |
| Sinuous Ridges in the Aeolis/Zephyria Region: ESP_020528_1750 ESP_020673_1750 (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 | -5.06 | 154. | 7.87 | 22.67 | 54.0 | 52.4 |
| Fan and Valley within Crater: ESP_020323_2050 ESP_020824_2050 (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 | 24.54 | 348. | -1.3 | 18.52 | 59.4 | 62.1 |
| Massif on the Floor of Coprates Chasma: ESP_020246_1680 ESP_020958_1680 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.1 | 296. | -6.3 | 10.26 | 56.4 | 51.3 |
| Very Fresh Northern Plains 6-Kilometer Diameter Crater: ESP_020156_2235 ESP_028714_2235 (Interval in Earth days: 666) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 43.24 | 225. | -1.5 | 8.405 | 64.1 | 58.9 |
| Well-Preserved 10-Kilometer Diameter Crater in Margaritifer Terra: ESP_020046_1600 ESP_020468_1600 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -19.6 | 356. | 4 | -13.5 | 58.4 | 56.8 |
| Wrinkle Ridges in East Meridiani Planum: ESP_020138_1845 ESP_020283_1845 (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 | 4.462 | 2.88 | -6.0 | 7.354 | 55.3 | 54.6 |
| Rayed Crater in Isidis Planitia: ESP_020240_1970 ESP_020952_1970 (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 | 16.88 | 95.6 | 3.08 | 17.82 | 56.4 | 59.3 |
| Active Geyser Locale: ESP_020241_0945 ESP_020242_0945 (Interval in Earth days: 0) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -85.4 | 103. | 8.72 | -13.9 | 87.4 | 89.5 |
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