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.
| 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 |
| Channel Head in Newton Crater: ESP_074356_1405 ESP_074923_1405 (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 | -38.9 | 202. | -2.9 | -17.9 | 48.7 | 42.6 |
| Small Delta or Fan: ESP_074435_1465 ESP_075292_1465 (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 | -33.2 | 205. | -7.5 | 6.888 | 47.4 | 36.9 |
| Confirm and Characterize Exit Breach and Compare to Channel: ESP_074485_1445 ESP_083017_1445 (Interval in Earth days: 665) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -35.1 | 280. | -2.2 | -22.6 | 46.5 | 52.5 |
| Ridges North of Vernal Crater: ESP_074693_1875 ESP_074983_1875 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.328 | 355. | -8.7 | 10.14 | 56.5 | 52.5 |
| Pole-Facing Gullies in 7-Kilometer Crater within Bond Crater: ESP_074457_1470 ESP_074747_1470 (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 | -32.7 | 323. | 1.02 | 17.64 | 46.5 | 41.4 |
| Light-Toned Deposits in Iani Chaos: ESP_074443_1790 ESP_074377_1790 (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 | -0.76 | 341. | 6.66 | 27.24 | 53.4 | 52.3 |
| Channel in Eastern Arabia Terra: ESP_074691_1800 ESP_075970_1800 (Interval in Earth days: 99) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.03 | 50.7 | -1.6 | 20.89 | 52.2 | 36.8 |
| Gully Monitoring: ESP_074437_1425 ESP_074859_1425 (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 | -36.9 | 150. | 3.50 | -23.4 | 46.8 | 43.5 |
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