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.
| 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 |
| Landslide Facing West near Cydonia Mensae: ESP_080456_2115 ESP_080522_2115 (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 | 31.37 | 347. | 12.1 | -5.83 | 47.5 | 49.5 |
| Streamlined Features in Athabasca Valles: ESP_080595_1890 ESP_080740_1890 (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 | 8.663 | 156. | 6.28 | 17.47 | 53.5 | 52.9 |
| Possible Dipping Layers in Ice-Affected Crater: ESP_080515_2115 ESP_080805_2115 (Interval in Earth days: 22) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 31.38 | 178. | -3.2 | 15.42 | 49.2 | 49.7 |
| Dune Ice Interaction West of Olympia Region: ESP_080570_2605 ESP_080333_2605 (Interval in Earth days: 19) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 80.45 | 96.7 | 2.25 | -15.3 | 63.1 | 62.0 |
| Light-Toned Exposures near Voeykov Crater: ESP_080340_1465 ESP_080274_1465 (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 | -33.0 | 283. | -1.3 | 15.81 | 77.0 | 76.2 |
| Ares Vallis: ESP_080549_1910 ESP_080760_1910 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 10.87 | 332. | 2.57 | -10.1 | 53.0 | 54.5 |
| 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 |
| Frost-Free Dunes in Viking 2 Image 544B05: ESP_080437_2570 ESP_080490_2570 (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 | 76.66 | 130. | 7.66 | -7.69 | 59.3 | 61.0 |
| Grooves and Cataracts in Eos Chasma: ESP_080576_1665 ESP_080431_1665 (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 | -13.3 | 318. | -0.6 | -16.6 | 64.1 | 65.6 |
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