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.
| Hillslope Morphologies in Crater: ESP_082945_1510 ESP_083011_1510 (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 | -28.8 | 83.4 | -4.8 | -26.4 | 51.8 | 52.7 |
| Sinuous Ridge between Craters: ESP_083008_1690 ESP_083641_1690 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.0 | 160. | 3.77 | -18.6 | 52.5 | 47.5 |
| Hebes Chasma Layered Deposits: ESP_083043_1790 ESP_083188_1790 (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 | -0.77 | 283. | 6.50 | 20.00 | 55.3 | 53.4 |
| Southern Canyon Wall in East Coprates Chasma: ESP_083029_1645 ESP_075974_1645 (Interval in Earth days: 549) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.3 | 305. | 22.5 | -8.66 | 49.9 | 35.2 |
| Ridges near Valley Network in Arabia Terra: ESP_083026_1885 ESP_083949_1885 (Interval in Earth days: 72) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.174 | 26.2 | 6.26 | -5.44 | 59.2 | 52.6 |
| Landslide in Crater in Arabia Terra: ESP_082935_1940 ESP_082869_1940 (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 | 13.68 | 350. | -0.2 | 23.3 | 62.5 | 60.7 |
| Athabasca Valles: ESP_083074_1895 ESP_083140_1895 (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 | 9.230 | 156. | -4.3 | -26.0 | 60.3 | 61.7 |
| Channel with Distinct Levees: ESP_083006_1575 ESP_083151_1575 (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 | -22.0 | 216. | 0 | 12.87 | 50.9 | 48.2 |
| Small Delta or Fan: ESP_083042_1885 ESP_083675_1885 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.626 | 309. | 6.05 | -18.1 | 59.4 | 56.7 |
| Well-Preserved 4-Kilometer Impact Crater: ESP_083095_1535 ESP_083240_1535 (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 | -26.2 | 307. | -5.3 | 9.499 | 49.9 | 46.9 |
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