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.
| Baetis Chasma: ESP_064645_1760 ESP_065410_1760 (Interval in Earth days: 60) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.19 | 295. | 8.33 | -23.4 | 56.7 | 56.9 |
| Floor of East Candor Chasma: ESP_064843_1730 ESP_064487_1730 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.89 | 291. | -8.7 | -23.9 | 57.4 | 59.4 |
| Network of Sinuous Ridges in Aeolis Dorsa: ESP_064848_1730 ESP_073039_1730 (Interval in Earth days: 638) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.70 | 154. | 4.51 | -24.5 | 56.4 | 60.0 |
| Light-Toned Knobby Unit in Degraded Crater: ESP_064772_1715 ESP_065260_1715 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.40 | 69.9 | -4.7 | -20.2 | 57.2 | 56.3 |
| Flow Features in Reull Vallis: ESP_064837_1405 ESP_065391_1405 (Interval in Earth days: 43) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.4 | 96.2 | 28.3 | 5.137 | 56.8 | 51.1 |
| Fractures and Inlet Valley : ESP_064798_1990 ESP_064653_1990 (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 | 18.64 | 76.2 | 0.85 | -16.8 | 62.7 | 63.1 |
| Fan-Shaped Deposit with Floor Outcrop in Camichel Crater: ESP_064750_1825 ESP_065304_1825 (Interval in Earth days: 43) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.468 | 308. | 4.35 | -28.4 | 57.9 | 60.2 |
| Nilosyrtis Mensae Dunes: ESP_064495_2150 ESP_064561_2150 (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 | 34.49 | 65.8 | 1.20 | -15.4 | 65.4 | 67.6 |
| Crater in Arabia Terra: ESP_064207_2205 ESP_064062_2205 (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 | 40.17 | 7.50 | 2.90 | -7.96 | 63.3 | 62.0 |
| Peace Vallis Channel in Gale Crater: ESP_064453_1760 ESP_064730_1760 (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 | -4.06 | 137. | 3.20 | -21.6 | 57.1 | 59.1 |
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