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.
| East Rim of Well-Preserved Impact Crater : ESP_028719_1615 ESP_028864_1615 (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 | -18.4 | 99.0 | -7.1 | 7.261 | 59.2 | 57.3 |
| Distorted Icy Terrain in Nilosyrtis Mensae Crater : ESP_028601_2145 ESP_028324_2145 (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 | 34.17 | 73.6 | -1.8 | 13.89 | 55.3 | 50.7 |
| Possible Repetitive Bedding Near Base of Central Lobe of Medusae Fossae : ESP_028650_1695 ESP_028795_1695 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -10.4 | 180. | 8.61 | 21.62 | 55.7 | 54.2 |
| Chevrons on Lava Surface in Marte Vallis : ESP_028716_1880 ESP_053704_1875 (Interval in Earth days: 1947) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.810 | 177. | 0 | 12.89 | 53.4 | 47.2 |
| Knobs and Troughs in Acidalia Planitia : ESP_028671_2115 ESP_035699_2115 (Interval in Earth days: 548) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 31.18 | 321. | 7.25 | 22.42 | 54.8 | 41.2 |
| Northeast Melas Chasma Dune Fields and Wall Rock : ESP_028857_1700 ESP_028923_1700 (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 | -10.0 | 290. | -4.8 | -26.4 | 56.1 | 57.7 |
| Erosional Morphologies in Lower Shalbatana Vallis : ESP_028869_1890 ESP_029291_1890 (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 | 8.738 | 319. | 6.05 | -5.96 | 53.6 | 56.4 |
| Fresh Small Rayed Crater : ESP_028629_1660 ESP_029051_1660 (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 | -13.9 | 34.4 | 8.94 | -9.1 | 56.9 | 56.5 |
| Proposed Future Landing Site in Arda Valles : ESP_028882_1600 ESP_028948_1600 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -19.6 | 327. | 7.83 | -15.0 | 57.5 | 58.8 |
| Layering in Graben Wall : ESP_028793_2265 ESP_072482_2265 (Interval in Earth days: 3404) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 45.91 | 229. | 0 | 24.14 | 61.8 | 55.9 |
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