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.
| Streamlined Landforms in Marte Vallis : ESP_044975_1885 ESP_045041_1885 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.463 | 177. | -1.4 | -19.3 | 47.2 | 48.6 |
| Double-Terraced Crater in Arcadia Planitia : ESP_044724_2270 ESP_044869_2270 (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 | 46.75 | 183. | 5.44 | 19.31 | 41.4 | 40.8 |
| Exposure of North Polar Layered Deposits : ESP_044783_2585 ESP_053341_2585 (Interval in Earth days: 666) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 78.57 | 1.01 | 0.17 | -19.9 | 57.0 | 57.3 |
| Plains North of Tempe Terra : ESP_044813_2320 ESP_045380_2320 (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 | 51.67 | 275. | -12. | 8.373 | 44.7 | 47.1 |
| Wrinkle Ridge and Channel Intersection along Huygens Crater Rim : ESP_044729_1600 ESP_045006_1600 (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 | -19.8 | 56.3 | -1.0 | -15.5 | 64.2 | 64.1 |
| Gullied Northern Crater in CTX Image: ESP_044680_2230 ESP_045458_2230 (Interval in Earth days: 61) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 42.50 | 308. | -23. | 1.189 | 43.2 | 45.5 |
| Streamlined Form in Lethe Vallis : ESP_044989_1845 ESP_045833_1845 (Interval in Earth days: 65) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.261 | 155. | 6.74 | -2.85 | 48.5 | 49.3 |
| Possible Gray Hematite in Capri Chasma : ESP_044891_1665 ESP_045313_1665 (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 | -13.3 | 313. | 1.73 | 14.11 | 59.2 | 56.8 |
| North Polar Barchan Dunes : ESP_044853_2580 ESP_045011_2580 (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 | 78.07 | 251. | -1.4 | 13.48 | 57.1 | 57.4 |
| Possible Chloride Deposit Disrupted By Simple Crater : ESP_044929_1495 ESP_052880_1495 (Interval in Earth days: 619) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -30.3 | 358. | 0 | 24.50 | 70.8 | 70.3 |
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