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.
| Candidate ExoMars Landing Site in Oxia Palus: ESP_040433_1985 ESP_048648_1985 (Interval in Earth days: 640) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.13 | 335. | 16.8 | -8.28 | 49.9 | 56.0 |
| Sinuous Ridge on the Orson Welles Bajada: ESP_039867_1805 ESP_032469_1805 (Interval in Earth days: 576) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.502 | 313. | -17. | -7.02 | 48.1 | 34.1 |
| Ares 3 Landing Site: The Martian Revisited: ESP_040776_2115 ESP_041277_2115 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 31.38 | 331. | -2.3 | 21.31 | 56.0 | 48.0 |
| Layers and Dark Dunes: ESP_039581_1520 ESP_049009_1520 (Interval in Earth days: 735) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.7 | 203. | -0.5 | 15.81 | 41.2 | 30.4 |
| Cerberus Palus Outlet Channel: ESP_039939_1810 ESP_040651_1810 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 1.216 | 146. | -1.3 | 15.96 | 46.5 | 37.2 |
| Topography in Region Dubbed Ithaca: ESP_040216_0950 ESP_040189_0950 (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 | -85.1 | 181. | 0.90 | 18.47 | 66.0 | 64.5 |
| Channel within Larger Channel in Northern Mid-Latitudes: ESP_039931_2165 ESP_048370_2165 (Interval in Earth days: 658) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.37 | 1.01 | -5.2 | 19.79 | 71.0 | 70.3 |
| Many-Layered Mantle in Hellas Planitia: ESP_039942_1370 ESP_040021_1370 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -42.8 | 70.5 | -0.4 | 25.67 | 39.4 | 37.0 |
| Candidate Landing Site for 2020 Mission in Hadriacus Palus: ESP_039968_1530 ESP_040034_1530 (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 | -26.9 | 78.0 | 2.41 | -20.6 | 36.8 | 38.0 |
| Crater in South Polar Layered Deposits: ESP_040057_0985 ESP_040571_0985 (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 | -81.4 | 189. | -2.7 | 11.88 | 61.9 | 66.0 |
Page 413 of 877 (8,766 images) | |||||