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.
| Large Polygons: ESP_034021_2400 ESP_042566_2400 (Interval in Earth days: 666) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 59.64 | 52.7 | -6.0 | 10.86 | 51.5 | 52.9 |
| Possible Glacial Cirque: ESP_033901_1390 ESP_042512_1390 (Interval in Earth days: 671) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -40.8 | 102. | -4.7 | 7.335 | 69.7 | 66.2 |
| Recent Crater: ESP_033733_2125 ESP_034234_2125 (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 | 32.16 | -0.3 | -3.7 | 21.40 | 40.9 | 38.4 |
| Shallow Crater with Cross-Cutting Valley: ESP_033880_2200 ESP_034882_2200 (Interval in Earth days: 78) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 39.46 | 305. | -4.8 | 23.57 | 42.8 | 39.0 |
| Channel in Ceraunius Fossae Region: ESP_033737_2040 ESP_034370_2040 (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 | 23.62 | 250. | 8.24 | -3.83 | 38.2 | 41.0 |
| Sinuous Ridges with Meanders and Scroll Bars in Aeolis Planum: ESP_034044_1740 ESP_034189_1740 (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 | -6.02 | 153. | 0.23 | 19.2 | 48.5 | 48.6 |
| Tilted Mesas Near Athabasca Valles: ESP_033965_1875 ESP_042576_1875 (Interval in Earth days: 671) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.490 | 148. | 0.31 | 13.81 | 41.9 | 39.4 |
| Possible Terraced Bullseye-Like Crater in Arcadia Planitia: ESP_033805_2285 ESP_034095_2285 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 47.93 | 191. | -5.8 | 15.43 | 46.9 | 43.5 |
| Two Craters along Floor and Wall of Mamers Valles: ESP_033851_2180 ESP_033917_2180 (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 | 37.79 | 15.9 | 9.04 | -7.19 | 41.2 | 42.3 |
| Possible Terraced Crater in Arcadia Planitia: ESP_033739_2290 ESP_034293_2290 (Interval in Earth days: 43) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 48.78 | 192. | -1.3 | -28.2 | 47.4 | 46.8 |
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