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.
Stratigraphy of Primary Mesa in Terby Crater: PSP_010826_1525 ESP_016272_1525 (Interval in Earth days: 424) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.1 | 74.2 | 4.13 | -10.0 | 65.9 | 60.7 |
Crater with Extensive Ejecta Deposits: PSP_010611_2210 ESP_027173_2210 (Interval in Earth days: 1290) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.51 | 175. | 0.50 | -12.9 | 54.2 | 44.1 |
Shalbatana Vallis: PSP_010461_1845 ESP_016619_1845 (Interval in Earth days: 480) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.397 | 315. | 0 | 0 | 54.7 | 45.8 |
Streamlined Landforms on Terraces of Ritchey Crater: PSP_010646_1510 ESP_016092_1510 (Interval in Earth days: 424) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -28.5 | 308. | 7.57 | -9.18 | 67.6 | 59.1 |
Very Fresh Small Crater at 48 North Latitude: PSP_010638_2280 ESP_051951_2280 (Interval in Earth days: 3219) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 47.60 | 157. | 2.16 | -18.8 | 56.3 | 43.7 |
High-Latitude Exposure of North Polar Layered Deposits: PSP_010555_2720 PSP_010583_2680 (Interval in Earth days: 3) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 87.91 | 156. | -8 | -8.54 | 75.6 | 75.2 |
Wallrock and Light-Toned Layering Geologic Contact in Coprates Chasma: ESP_011385_1695 ESP_011451_1695 (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 | -10.2 | 290. | -2.8 | -24.8 | 58.4 | 60.0 |
Central Peak of Gale Crater: PSP_010428_1745 ESP_016085_1745 (Interval in Earth days: 440) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.40 | 137. | 4.52 | -23.3 | 57.8 | 46.9 |
Large Clay and Chloride Exposure in Southeast Sirenum Fossae Region: PSP_010900_1405 ESP_016201_1405 (Interval in Earth days: 413) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.4 | 216. | -5.2 | -28.4 | 71.9 | 69.5 |
Possible MSL Landing Site in Gale Crater: ESP_011417_1755 ESP_011562_1755 (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 | -4.44 | 137. | -15. | 1.284 | 58.8 | 57.4 |
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