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.
| Outcrop in Athabasca Valles Lava: ESP_082705_1880 ESP_082270_1880 (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 | 7.779 | 149. | 27.6 | 7.677 | 57.8 | 59.0 |
| Contact between Medusae Fossae and Northern Flank of Apollinaris Mons: ESP_082757_1725 ESP_082322_1725 (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 | -7.26 | 173. | 6.07 | -7.55 | 55.1 | 58.2 |
| Small Sinuous Ridge at Base of Small Hill in Aeolis Dorsa: ESP_082560_1735 ESP_082771_1735 (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 | -6.46 | 153. | 0.76 | -24.1 | 56.7 | 57.7 |
| Complex Crater near Streamlined Feature in Bahram Vallis: ESP_082673_1970 ESP_082963_1970 (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 | 16.79 | 304. | 7.69 | 19.83 | 63.0 | 62.5 |
| Layered Deposits in Burroughs Crater: ESP_082720_1075 ESP_082878_1075 (Interval in Earth days: 13) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -72.4 | 117. | 0.60 | 21.39 | 67.4 | 63.2 |
| Ridges and Fractures in Sublimation-Pit Crater with Hale Crater Ejecta: ESP_082620_1415 ESP_082844_1415 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.0 | 319. | -7.3 | 22.81 | 57.5 | 51.8 |
| Ancient Crust Outcrops in Coprates Chasma: ESP_082515_1650 ESP_082594_1650 (Interval in Earth days: 7) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.9 | 304. | -14. | 15.33 | 57.4 | 54.4 |
| Impact Crater and Ejecta: ESP_082677_1910 ESP_083244_1910 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 11.00 | 196. | -8.7 | -26.0 | 62.0 | 62.0 |
| Layered Deposits in Liais Crater: ESP_082694_1045 ESP_082681_1045 (Interval in Earth days: 1) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -75.4 | 106. | 8.06 | -8.39 | 68.8 | 70.2 |
| Exposure of Eroded Fan Deposits: ESP_082858_1655 ESP_082647_1655 (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 | -14.4 | 298. | -18. | 4.844 | 54.9 | 54.9 |
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