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.
| Floor of Cut Crater: ESP_016461_1680 ESP_025533_1680 (Interval in Earth days: 707) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.8 | 312. | -6.7 | 15.71 | 53.1 | 53.0 |
| Layers Exposed in Wall of Crater in the Floor of Hydaspis Chaos: ESP_016513_1850 ESP_017502_1850 (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 | 5.146 | 329. | 3.09 | -12.0 | 44.4 | 51.1 |
| Volcanic Features in Ceraunius Fossae Region: ESP_016661_2020 ESP_017096_2020 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.86 | 248. | -16. | 25.35 | 42.3 | 40.1 |
| Gale Crater Layers in Northeast Section of Mound with Possible Sulfates: ESP_016586_1755 ESP_016731_1755 (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 | -4.64 | 138. | 0.77 | 18.24 | 49.8 | 49.8 |
| Possible MSL Landing Site in Syrtis Major: ESP_016364_1980 ESP_016219_1980 (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 | 17.89 | 77.2 | -14. | -27.6 | 41.5 | 42.2 |
| Chaos on the Floor of Candor Chasma: ESP_016686_1735 ESP_017108_1735 (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 | -6.49 | 287. | 10.2 | -4.71 | 51.1 | 55.2 |
| Terrain South of Newcomb Crater: ESP_016736_1520 ESP_068970_1525 (Interval in Earth days: 4070) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.6 | 5.59 | 4.65 | -7.50 | 65.7 | 63.9 |
| Fresh Multiple Impact: ESP_016718_2005 ESP_018353_2005 (Interval in Earth days: 127) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 20.26 | 131. | 0.06 | 15.40 | 41.3 | 44.6 |
| Zunil Crater Secondary Crater Cluster: ESP_016796_1830 ESP_016941_1830 (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 | 2.871 | 164. | -8.6 | 7.724 | 48.3 | 48.1 |
| Fresh Crater on Alba Patera: ESP_016371_2235 ESP_016226_2235 (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 | 43.05 | 240. | 4.58 | -7.09 | 43.2 | 44.8 |
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