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.
| Small Fresh Impact Crater: ESP_036067_1825 ESP_036423_1825 (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 | 2.498 | 2.70 | -8.8 | 14.78 | 54.5 | 53.0 |
| Chasma Boreale Gypsum Dunes: ESP_036330_2650 ESP_036634_2650 (Interval in Earth days: 24) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 84.98 | 339. | 4.08 | -11.2 | 64.0 | 68.0 |
| Candidate Landing Site for 2020 Mission in Kashira Crater: ESP_036358_1525 ESP_052116_1525 (Interval in Earth days: 1228) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.0 | 341. | -0.2 | -22.1 | 70.7 | 65.9 |
| Crater Exposing Layers Filling Larger Crater: ESP_036302_1745 ESP_069970_1745 (Interval in Earth days: 2623) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.46 | 67.5 | 4.31 | -4.72 | 57.7 | 61.2 |
| North Polar Barchan Dunes Dubbed Caladan: ESP_036279_2540 ESP_036081_2540 (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 | 73.63 | 328. | -21. | -7.95 | 58.8 | 56.1 |
| Irregular Mesa in Northern Elysium Planitia: ESP_036206_1935 ESP_036351_1935 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 13.10 | 166. | -7.1 | 13.77 | 50.1 | 48.8 |
| Well-Preserved Crater with Central Uplift and Layered Ejecta: ESP_036011_1650 ESP_045598_1650 (Interval in Earth days: 747) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.9 | 93.2 | -5.5 | 9.012 | 64.1 | 56.9 |
| Sinus Meridiani and Meridiani Planum Stratigraphy: ESP_036146_1840 ESP_037346_1840 (Interval in Earth days: 93) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.077 | 5.74 | -6.5 | -25.8 | 53.6 | 57.5 |
| Branched and Curving Ridges among Yardangs: ESP_036167_1730 ESP_046031_1730 (Interval in Earth days: 769) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.75 | 152. | 5.51 | -24.7 | 58.4 | 54.6 |
| Crater with Steep Slopes: ESP_036235_2170 ESP_042499_2170 (Interval in Earth days: 489) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.59 | 90.8 | 4.32 | -21.5 | 45.1 | 44.1 |
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