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.
| Marte Vallis Streamlined Landforms: ESP_016202_1895 ESP_016835_1895 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.254 | 179. | 5.93 | -8.19 | 40.6 | 45.8 |
| Well-Preserved Impact Crater: ESP_015905_2235 ESP_016182_2235 (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 | 42.91 | 3.36 | 3.72 | -15.9 | 45.9 | 45.8 |
| Crater Rim Gullies Filled with Small Dunes: ESP_015934_2165 ESP_037243_2165 (Interval in Earth days: 1660) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.09 | 292. | 1.58 | -16.4 | 42.8 | 56.6 |
| Stranded Lobe of Material with Associated Ridge on Valley Floor: ESP_016238_2180 ESP_017161_2180 (Interval in Earth days: 72) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 37.54 | 273. | -3.4 | 6.789 | 42.5 | 40.5 |
| Gullied Crater Wall: ESP_015950_1395 ESP_016451_1395 (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 | -40.3 | 225. | 4.65 | 25.21 | 64.5 | 70.3 |
| Cerberus Fossae Cutting Hill: ESP_016229_1895 ESP_016862_1895 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.130 | 162. | 4.10 | -9.74 | 40.9 | 46.1 |
| Possible Phyllosilicate-Rich Terrain: ESP_016102_2160 ESP_044044_2160 (Interval in Earth days: 2177) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.47 | 26.3 | 2.45 | 19.39 | 42.0 | 37.7 |
| Mounds on Hrad Vallis Mudflow: ESP_016256_2155 ESP_016322_2155 (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 | 35.06 | 142. | -2.8 | -19.2 | 41.7 | 43.0 |
| Juventae Region Mound and Possible Sulfate-Rich Terrain: ESP_015934_1760 ESP_016646_1760 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.74 | 298. | 0 | 21.43 | 42.9 | 48.4 |
| Crater with Rampart-Like Ejecta Exposed in Cross Section: ESP_016080_1745 ESP_025574_1745 (Interval in Earth days: 740) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.30 | 272. | 0 | 11.85 | 45.1 | 49.7 |
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