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.
| Ceraunius Fossae: ESP_028001_2070 ESP_053688_2070 (Interval in Earth days: 2001) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 26.57 | 253. | 5.82 | -5.11 | 47.6 | 42.7 |
| Small Shield in Tharsis Region Embayed by Younger Lavas: ESP_027988_2010 ESP_033658_2010 (Interval in Earth days: 442) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 20.48 | 248. | 5.19 | -6.24 | 47.9 | 39.0 |
| Alcove Sourcing Alluvial Fan in Crater: ESP_027863_1670 ESP_028351_1670 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.7 | 65.7 | -0.7 | -19.6 | 59.7 | 59.5 |
| Multiple Unconformities in North Polar Layered Deposits: ESP_028022_2595 ESP_027903_2595 (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 | 79.28 | 28.0 | -8.9 | 6.864 | 66.8 | 64.2 |
| Flow Boundary in Elysium Planitia: ESP_028149_2085 ESP_028215_2085 (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 | 28.29 | 172. | 4.18 | -12.8 | 49.0 | 51.1 |
| Possible Future Landing Site in Cerberus Palus: ESP_028005_1870 ESP_034532_1870 (Interval in Earth days: 509) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 6.749 | 146. | 5.47 | 26.39 | 50.8 | 44.3 |
| Change Detection of Aprons of Icy Material Draping North Polar Scarp: ESP_027924_2650 ESP_027806_2650 (Interval in Earth days: 9) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 85.06 | 147. | 9.23 | -4.68 | 68.4 | 67.4 |
| Fractures in Chryse Planitia: ESP_027959_1990 ESP_028737_1990 (Interval in Earth days: 60) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.71 | 321. | -5.3 | 7.285 | 48.9 | 53.3 |
| Extensive Outcrops of Rhythmic Stratigraphy in Arabia Region Crater: ESP_028129_1905 ESP_028195_1905 (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 | 10.35 | 1.11 | 4.69 | -15.4 | 50.4 | 52.2 |
| High-Latitude Exposure of North Polar Layered Deposits: ESP_028001_2680 ESP_019286_2680 (Interval in Earth days: 679) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 87.93 | 205. | -13. | -22.6 | 72.3 | 74.2 |
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