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.
| Potential Compound Dune in USGS Dune Database 1687-642: ESP_092317_1155 ESP_092383_1155 (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 | -64.2 | 168. | 0.25 | -14.7 | 52.1 | 52.5 |
| Streamlined Shapes South of Harmakhis Vallis: ESP_092425_1385 ESP_092636_1385 (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 | -41.0 | 93.9 | 2.97 | -20.3 | 42.5 | 42.2 |
| Triangular Scars on Hillslopes: ESP_092549_1335 ESP_092325_1335 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -46.2 | 308. | 3.67 | -16.2 | 42.4 | 46.3 |
| Holden Crater Sedimentary Fan: ESP_092456_1525 ESP_092667_1525 (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 | -26.9 | 325. | 0.76 | -25.0 | 41.6 | 41.2 |
| Network of Channels on Rim of Newton Crater: ESP_092632_1420 ESP_092698_1420 (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 | -37.6 | 200. | -2.6 | -25.5 | 40.1 | 41.4 |
| Banded or Layered Megabreccia Clasts in Nili Fossae: ESP_092544_1995 ESP_092610_1995 (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 | 19.17 | 76.5 | -1.1 | -26.7 | 61.3 | 62.3 |
| Inverted Channel in Noachis Terra: ESP_092678_1610 ESP_092177_1610 (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 | -18.9 | 22.8 | -12. | 8.654 | 41.2 | 45.8 |
| Alluvial Fan in Kasei Vallis: ESP_092602_2030 ESP_092681_2030 (Interval in Earth days: 7) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 22.70 | 292. | -2.3 | 24.40 | 63.3 | 61.0 |
| Possible Eroded Dyke System in Atlantis Chaos: ESP_092593_1450 ESP_092224_1450 (Interval in Earth days: 29) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -34.7 | 183. | 17.5 | -7.74 | 38.6 | 45.1 |
| Triangular Scars on Hillslopes: ESP_092443_1320 ESP_092021_1320 (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 | -47.7 | 326. | -24. | -7.02 | 46.0 | 50.0 |
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