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.
| Valleys near Huygens Crater: ESP_074796_1645 ESP_075007_1645 (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 | -15.3 | 64.7 | 7.34 | -6.67 | 44.1 | 42.6 |
| Variety of Spider Terrain: ESP_075003_0995 ESP_074911_0995 (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 | -80.6 | 189. | 8.97 | -8.06 | 59.8 | 61.0 |
| Mesa Stratigraphy at Terby Crater: ESP_074743_1520 ESP_075376_1520 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.5 | 73.8 | 3.18 | -17.5 | 42.8 | 37.9 |
| Small Delta or Fan: ESP_074787_1945 ESP_075499_1945 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 14.57 | 308. | -9.4 | 15.83 | 60.1 | 50.8 |
| Cliffs of Ice: ESP_074914_1225 ESP_074980_1225 (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 | -57.1 | 89.7 | 1.33 | -12.8 | 47.0 | 47.6 |
| On Bond Crater’s Northern Slope: ESP_074246_1475 ESP_074391_1475 (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 | -32.1 | 323. | 8.54 | 21.18 | 48.8 | 45.8 |
| Colorful Rocks Exposed in a Fresh Impact Crater: ESP_074332_1580 ESP_075400_1580 (Interval in Earth days: 83) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -21.9 | 135. | -8.5 | 6.111 | 49.4 | 36.2 |
| Drainage Divide Migration in Tyrrhena Terra: ESP_074439_1525 ESP_075296_1525 (Interval in Earth days: 67) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -26.9 | 94.7 | -1.5 | 13.67 | 47.1 | 36.1 |
| Steep Southern Coprates Chasma Wall Slopes: ESP_074392_1655 ESP_074814_1655 (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 | -14.1 | 296. | -0.4 | -28.8 | 49.6 | 47.1 |
| Armored Ejecta Deposits with Mafic Signature: ESP_074414_1195 ESP_074335_1195 (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 | -60.0 | 62.1 | 5.72 | -15.4 | 53.2 | 55.9 |
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