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.
| Gullies and Lobate Material in a Crater in the Nereidum Montes: ESP_014127_1420 ESP_020786_1420 (Interval in Earth days: 519) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.5 | 314. | -2.1 | 19.93 | 37.6 | 54.3 |
| Faulting in South Polar Layered Deposits: ESP_012762_1070 ESP_013171_1070 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -72.9 | 146. | 10.3 | -12.8 | 58.0 | 56.3 |
| Rayed Crater: ESP_013955_1020 ESP_013968_1020 (Interval in Earth days: 1) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -77.8 | 345. | -6.7 | 7.228 | 62.3 | 61.6 |
| 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 |
| 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 |
| 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 |
| Nili Fossae-NE Syrtis Phyllosilicate-Sulfate Stratigraphy: ESP_013041_1975 ESP_030025_1975 (Interval in Earth days: 1324) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.42 | 76.9 | -3.2 | 12.81 | 61.2 | 60.4 |
| 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 |
| Well Preserved 20 Kilometer Diameter Impact Crater: ESP_013684_1455 ESP_020910_1455 (Interval in Earth days: 563) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -34.0 | 168. | -2.8 | 19.71 | 36.4 | 51.7 |
| Layered Bedrock in Northeast Hellas Planitia: ESP_013964_1490 ESP_020267_1490 (Interval in Earth days: 491) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -30.7 | 82.9 | 1.84 | 19.77 | 34.9 | 58.9 |
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