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.
| Wrinkle Ridge and Channel Intersection : ESP_059243_1440 ESP_059388_1440 (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 | -35.7 | 180. | -8.2 | 5.95 | 47.3 | 49.0 |
| Well-Preserved Crater in Kasei Valles : ESP_059436_2105 ESP_060069_2105 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 30.35 | 302. | -2.8 | -13.4 | 41.7 | 39.8 |
| Monitor Opposing Barchan Dunes and Star Dunes : ESP_059292_1310 ESP_058646_1310 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -48.4 | 282. | 14.4 | -8.91 | 56.3 | 46.8 |
| Lava Flows Embaying Impact Crater: ESP_059452_1540 ESP_076135_1540 (Interval in Earth days: 1300) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -25.9 | 232. | -0.5 | -15.5 | 44.0 | 37.4 |
| Gullied Crater Wall : ESP_059242_1335 ESP_066983_1335 (Interval in Earth days: 603) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -46.1 | 208. | 1.75 | 17.62 | 54.3 | 42.8 |
| Well-Preserved Small Impact Crater on Hellas Planitia Floor : ESP_059261_1380 ESP_067886_1380 (Interval in Earth days: 672) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -41.7 | 49.7 | -4.4 | 21.24 | 51.7 | 52.2 |
| Possible Olivine-Rich Crater in Terra Sirenum : ESP_059322_1515 ESP_076783_1515 (Interval in Earth days: 1361) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -28.2 | 182. | -5.0 | 23.12 | 43.6 | 42.7 |
| Gullies on Outer Crater Wall in Nereidum Montes : ESP_059357_1385 ESP_058935_1385 (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 | -41.0 | 307. | 5.31 | 18.04 | 52.3 | 44.5 |
| Ancient Bedforms on Gordii Dorsum : ESP_059268_1895 ESP_059545_1895 (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 | 9.495 | 210. | 6.39 | -21.1 | 33.0 | 35.9 |
| Fractured Ground in Aram Chaos : ESP_059237_1830 ESP_059382_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 | 2.925 | 339. | -8.7 | 7.4 | 33.2 | 32.5 |
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