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.
| Features around Crater in Terra Sabaea: ESP_089842_2165 ESP_089565_2165 (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 | 36.09 | 50.5 | -24. | -6.66 | 54.5 | 50.2 |
| Light-Toned Exposures on Floor of Coprates Chasma: ESP_089780_1645 ESP_090057_1645 (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 | -15.2 | 306. | 6.84 | -14.8 | 62.3 | 62.9 |
| Inverted Valley and Rings in Erebus Montes: ESP_089718_2210 ESP_090061_2210 (Interval in Earth days: 26) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.86 | 188. | 26.6 | -1.13 | 49.3 | 55.9 |
| Moraine-Like Assemblage Exposed by Ice Retreat: ESP_089855_2215 ESP_090422_2215 (Interval in Earth days: 45) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.98 | 51.3 | 6.63 | 23.73 | 52.7 | 58.7 |
| Barchan to Sand Sheet Transition in Central Herschel Crater: ESP_089892_1655 ESP_090037_1655 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.1 | 129. | -3.4 | 17.28 | 62.1 | 60.1 |
| Iani Chaos: ESP_089660_1780 ESP_089238_1780 (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 | -1.75 | 341. | -6.6 | 6.11 | 57.5 | 56.6 |
| Potential Rotorcraft Landing Site Characterization: ESP_089771_2185 ESP_089837_2185 (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 | 38.22 | 186. | -8.1 | -22.4 | 52.6 | 54.7 |
| Dune Interaction with Residual Polar Ice: ESP_089800_2600 ESP_089826_2600 (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 | 79.64 | 98.5 | -0.5 | 16.96 | 67.8 | 67.0 |
| Crater in Arabia Terra: ESP_089804_2205 ESP_090160_2205 (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 | 39.96 | 7.23 | -21. | -7.62 | 54.5 | 57.6 |
| Glacier Layering Revealed by Impact Crater on Viscous Flow Features Surface: ESP_089764_2200 ESP_089487_2200 (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 | 39.61 | 17.6 | -8.7 | 10.06 | 52.8 | 48.4 |
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