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.
| Vent and Fissure System East of Olympus Mons: ESP_064700_1975 ESP_064555_1975 (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 | 17.54 | 233. | -14. | -29.2 | 62.9 | 63.2 |
| Gully Monitoring: ESP_064726_1390 ESP_065491_1390 (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 | -40.8 | 249. | -0.4 | -21.8 | 61.0 | 52.1 |
| 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 |
| 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 |
| Channels with Tributaries on Rocky Plains Northwest of Argyre Region: ESP_064645_1320 ESP_082568_1320 (Interval in Earth days: 1397) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -47.5 | 301. | 5.97 | -6.62 | 63.9 | 60.6 |
| 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 |
| Smooth Area in Phlegra Montes: ESP_064531_2155 ESP_064465_2155 (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 | 35.29 | 164. | -8.4 | 8.287 | 67.0 | 64.8 |
| Small Barchan Dunes in Northeast Argyre Region: ESP_064789_1350 ESP_064723_1350 (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 | -44.6 | 331. | -5.9 | 10.38 | 61.7 | 61.4 |
| Inverted Channels: ESP_064527_1440 ESP_055573_1440 (Interval in Earth days: 698) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -35.6 | 280. | 9.24 | -8.74 | 61.2 | 60.4 |
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