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.
| Dark Dunes and Aeolian Units in Melas Chasma : ESP_057551_1675 ESP_057894_1675 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.2 | 289. | -3.5 | -14.3 | 36.9 | 34.1 |
| South Polar Layered Deposits : ESP_057666_0920 ESP_057678_0920 (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 | -87.7 | 82.2 | 13.8 | 27.19 | 65.8 | 64.8 |
| Valleys in Central Pit Crater Northwest of Hellas Planitia : ESP_057613_1580 ESP_057547_1580 (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 | -21.7 | 38.2 | -4.1 | 11.23 | 33.8 | 33.3 |
| Scarp in Mid-Latitudes : ESP_057809_1215 ESP_057598_1215 (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 | -58.0 | 93.6 | 8.05 | -2.79 | 44.0 | 44.2 |
| Slope Features in Arabia Terra : ESP_057878_2115 ESP_058010_2115 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 31.17 | 356. | 23.5 | 2.71 | 59.8 | 59.1 |
| Crater with Spiders and Polygons : ESP_057520_1015 ESP_057467_1015 (Interval in Earth days: 4) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -78.2 | 73.0 | -1.5 | 15.60 | 58.1 | 57.0 |
| Contributory Channels Over Syrtis Major Lava Flows : ESP_057717_1940 ESP_057651_1940 (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 | 13.65 | 75.8 | -7.8 | 6.834 | 49.9 | 49.9 |
| Dark Sediments in Medusae Fossae Formation : ESP_057635_1795 ESP_057701_1795 (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 | -0.64 | 154. | 7.71 | -7.69 | 40.7 | 40.9 |
| Lava Flowing into Impact Crater in Elysium Planitia : ESP_057648_1870 ESP_074476_1870 (Interval in Earth days: 1311) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 6.844 | 158. | 5.84 | 19.33 | 45.3 | 55.9 |
| Layering in Burroughs Crater : ESP_057716_1080 ESP_057848_1080 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -71.7 | 118. | -1.5 | -11.2 | 53.9 | 55.3 |
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