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.
| Crossing Wrinkle Ridges in Tyrrhena Dorsa: ESP_012631_1555 PSP_005234_1555 (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 | -24.1 | 115. | -1.3 | 17.00 | 48.2 | 31.9 |
| Cratered Cones in Galaxias Colles: ESP_012946_2165 ESP_013236_2165 (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 | 36.17 | 147. | 4.76 | 26.24 | 74.0 | 71.2 |
| Basal Exposure of South Polar Layered Deposits: ESP_013290_1075 ESP_013092_1075 (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 | -72.2 | 138. | -18. | 5.428 | 55.8 | 55.0 |
| Marte Vallis Streamlined Landforms: ESP_014092_1955 ESP_014158_1955 (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 | 15.46 | 183. | -6.8 | -25.9 | 48.1 | 48.6 |
| Warrego Valles Headwater Region: ESP_013153_1390 ESP_013298_1390 (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 | -40.6 | 266. | -5.4 | 6.316 | 42.0 | 39.7 |
| Western Slope of Asimov Crater: ESP_013110_1325 ESP_013611_1325 (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 | -47.0 | 4.17 | -23. | -7.91 | 45.4 | 41.0 |
| Possible Clay and Sulfate in Terra Sirenum Layered Deposit: ESP_013485_1535 ESP_013907_1535 (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 | -26.0 | 199. | 4.43 | -12.0 | 36.9 | 35.3 |
| Athabasca Valles Flood Erosion of Impact Crater: ESP_012959_1895 ESP_013104_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 | 9.328 | 155. | 4.51 | 21.68 | 56.5 | 54.0 |
| Trough in Phoenicis Lacus: ESP_013971_1675 ESP_014327_1675 (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 | -12.2 | 249. | -2.9 | 9.647 | 35.6 | 32.9 |
| Exposure of South Polar Layered Deposits with Minor Faulting: ESP_012855_1065 ESP_012723_1065 (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 | -73.2 | 132. | -7.1 | 7.21 | 58.4 | 58.8 |
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