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.
| Megadunes in Hyperborei Cavi: ESP_089212_2620 ESP_089238_2620 (Interval in Earth days: 2) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 82.03 | 312. | -8.3 | 5.626 | 62.8 | 62.2 |
| Layering in Southern Lucus Planum: ESP_089336_1720 ESP_089481_1720 (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 | -7.84 | 187. | 4.06 | 19.82 | 59.8 | 58.4 |
| Layering in Lucus Planum: ESP_089244_1710 ESP_089521_1710 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.00 | 178. | 8.29 | -21.2 | 60.3 | 61.9 |
| Light-Toned Exposures in Capri Chasma: ESP_089582_1665 ESP_089437_1665 (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 | -13.1 | 312. | -0.7 | -17.4 | 62.4 | 64.0 |
| Avalanche Scarp: ESP_089280_2640 ESP_089386_2640 (Interval in Earth days: 8) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 83.76 | 236. | 6.42 | -8.01 | 63.6 | 65.4 |
| Possible Sulfate-Rich Deposit: ESP_089319_1730 ESP_089741_1730 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.16 | 291. | 5.45 | -5.79 | 59.4 | 59.6 |
| Channelized Flow in Arcadia Planitia: ESP_089587_2285 ESP_089455_2285 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 48.17 | 169. | -17. | 9.076 | 53.4 | 49.7 |
| Features around Crater in Terra Sabaea: ESP_089319_2205 ESP_089385_2205 (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 | 39.93 | 284. | 8.56 | -7.88 | 47.1 | 49.1 |
| Curve in Valley in Northern Terra Cimmeria: ESP_089390_1675 ESP_089535_1675 (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 | -12.4 | 154. | -8.8 | 8.148 | 63.0 | 61.6 |
| Light-Toned Mesas in Arcadia Planitia: ESP_089560_2260 ESP_089336_2260 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 45.44 | 183. | 12.9 | -21.3 | 49.9 | 50.8 |
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