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.
| Lower of Two Inner Channels in Southeast Kasei Valles: ESP_026536_2015 ESP_027670_2015 (Interval in Earth days: 88) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 20.95 | 287. | -9.8 | 21.55 | 43.9 | 44.7 |
| Well-Preserved Impact Crater: ESP_026238_1520 ESP_053692_1525 (Interval in Earth days: 2140) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.9 | 149. | -6.6 | 13.05 | 70.5 | 69.2 |
| Proximal Region of Athabasca Valles: ESP_026554_1900 ESP_019829_1900 (Interval in Earth days: 524) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.961 | 157. | -5.2 | 1.324 | 47.9 | 53.4 |
| Sharp-Rimmed Crater on Northern Plains: ESP_026383_2465 ESP_026673_2465 (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 | 66.00 | 137. | -7.2 | 4.831 | 49.1 | 48.3 |
| Impact Crater on East Side of Gale Crater: ESP_026502_1750 ESP_026647_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 | 138. | -3.6 | 13.91 | 55.8 | 55.0 |
| Eastern Rim and Ejecta of Crater in Margaritifer Terra: ESP_026257_1605 ESP_026402_1605 (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 | -19.2 | 348. | -0.9 | 15.10 | 64.1 | 63.8 |
| Channeled Features as Seen in CTX Image B21_017629_1522: ESP_026345_1500 ESP_026833_1500 (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 | -29.9 | 105. | 21.6 | -7.04 | 70.9 | 73.4 |
| Heavily Dissected Ancient Bedrock: ESP_026319_1740 ESP_062846_1740 (Interval in Earth days: 2846) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.17 | 94.7 | -3.5 | -16.0 | 55.9 | 58.6 |
| Exposed Bedrock in Crater Central Uplift off Thaumasia Planum: ESP_026496_1610 ESP_027485_1610 (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 | -19.0 | 304. | -6.5 | 5.269 | 65.1 | 64.1 |
| Light-Toned Layering along Floor of Small Trough Near Juventae Chasma: ESP_026272_1730 ESP_026628_1730 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.84 | 298. | -5.3 | 6.566 | 56.2 | 56.6 |
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