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.
| Faulted Layered Deposits in Capen Crater: ESP_021588_1870 ESP_022656_1870 (Interval in Earth days: 83) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 6.690 | 14.0 | 5.10 | 28.80 | 54.4 | 41.7 |
| Uplifted Bedrock in the Central Peak of an Impact Crater: ESP_020929_1360 ESP_021707_1360 (Interval in Earth days: 60) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -43.4 | 12.6 | 3.88 | -7.43 | 55.0 | 44.1 |
| Mesa in Acidalia Planitia: ESP_020587_2250 ESP_047105_2250 (Interval in Earth days: 2066) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 44.76 | 338. | 0.81 | 27.13 | 71.0 | 67.9 |
| Aeolian Change Detection in Trouvelot Crater: ESP_020956_1955 ESP_020811_1955 (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 | 15.33 | 346. | 16.4 | 0.7 | 58.8 | 59.5 |
| 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 |
| Fresh Impact Crater with Gullies and Bedrock: ESP_020950_1410 ESP_020884_1410 (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 | -38.5 | 159. | -5.5 | 13.36 | 54.1 | 53.6 |
| 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 |
| Channels and Lava Flows: ESP_020472_2010 ESP_028384_2010 (Interval in Earth days: 617) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 20.54 | 241. | -6.5 | -28.5 | 59.8 | 53.7 |
| Light-Toned Layering in Ladon Valles: ESP_020759_1595 ESP_029238_1595 (Interval in Earth days: 660) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -20.3 | 329. | 13.8 | -4.99 | 52.3 | 56.2 |
| Well-Preserved 6-Kilometer Diameter Crater: ESP_020807_2055 ESP_021664_2055 (Interval in Earth days: 67) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 25.33 | 94.6 | 0.74 | 22.70 | 63.6 | 64.3 |
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