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.
| Rock Glacier-Like Feature: ESP_092547_1380 ESP_092758_1380 (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 | -41.5 | 1.56 | 8.51 | -12.4 | 40.9 | 40.6 |
| 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 |
| 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 |
| Features in Nepenthes Mensae: ESP_092305_1920 ESP_092384_1920 (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 | 11.99 | 124. | -0.9 | 24.20 | 58.6 | 56.3 |
| 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 |
| 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 |
| Channel Breach: ESP_092311_1950 ESP_092034_1950 (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 | 15.01 | 320. | 4.46 | 25.66 | 60.1 | 60.0 |
| Channel Leading to Crater in Terra Cimmeria: ESP_092594_1695 ESP_092805_1695 (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 | -10.5 | 154. | 0.42 | -22.8 | 43.9 | 43.2 |
| Thermal Anomaly in Young Lava Flows of Elysium Mons: ESP_092633_1960 ESP_092989_1960 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 15.59 | 165. | 13.9 | 2.663 | 57.1 | 53.8 |
| Kasei Valles Flood Grooves and Chaotic Terrain: ESP_092655_1930 ESP_092866_1930 (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 | 12.74 | 285. | 3.94 | -16.4 | 55.6 | 54.5 |
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