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.
| Dune Interaction with Residual Polar Ice: ESP_080398_2605 ESP_079884_2605 (Interval in Earth days: 40) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 80.56 | 98.8 | 21.6 | 8.03 | 60.3 | 57.7 |
| Dune Interaction with Residual Polar Ice: ESP_080372_2605 ESP_080280_2605 (Interval in Earth days: 7) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 80.58 | 98.0 | 7.78 | -6.43 | 60.8 | 61.0 |
| Streamlined Landforms adjacent to Shalbatana Vallis: ESP_080299_1895 ESP_080444_1895 (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 | 9.172 | 318. | -13. | 12.02 | 54.3 | 52.6 |
| Terrain Sample in Cydonia Region: ESP_080535_2210 ESP_080970_2210 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.76 | 350. | 0 | 24.49 | 49.3 | 51.2 |
| Aram Chaos: ESP_080285_1830 ESP_080351_1830 (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 | 2.757 | 338. | 16.3 | -2.05 | 54.8 | 56.3 |
| Traverse Ramp in East Coprates Chasma: ESP_080405_1640 ESP_079983_1640 (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 | -15.8 | 307. | -4.1 | -14.2 | 66.2 | 67.4 |
| Region adjacent to Zhurong Rover Landing Site: ESP_080201_2055 ESP_080346_2055 (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 | 25.18 | 109. | -0.3 | 20.25 | 48.1 | 46.9 |
| Curvilinear Ridges on Floor of Shalbatana Vallis: ESP_080589_1885 ESP_080233_1885 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.367 | 318. | 19.4 | -1.16 | 52.6 | 53.6 |
| Lava Filling Craters in Elysium Planitia: ESP_080529_1895 ESP_080674_1895 (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 | 9.230 | 159. | -7.8 | 3.279 | 54.3 | 53.7 |
| Eroded Sedimentary Rock Layers: ESP_080568_1670 ESP_080779_1670 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.7 | 176. | -1.1 | -14.0 | 63.8 | 64.2 |
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