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.
| Fresh 500-meter Diameter Impact Crater: ESP_084408_1745 ESP_085199_1745 (Interval in Earth days: 62) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.54 | 93.1 | -3.5 | 19.38 | 39.7 | 33.7 |
| Streamline Feature Surrounding Crater in Ares Vallis: ESP_084162_1985 ESP_084373_1985 (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 | 18.12 | 327. | -2.4 | -21.9 | 56.4 | 55.0 |
| Phlegra Montes: ESP_084471_2160 ESP_084682_2160 (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 | 35.82 | 163. | 29.5 | 13.04 | 63.8 | 61.8 |
| Landforms above Subsurface Radar Observations of South Polar Cap: ESP_084261_0935 ESP_084247_0935 (Interval in Earth days: 1) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -86.5 | 200. | 0.09 | 14.22 | 67.1 | 65.7 |
| Crater: ESP_084392_1205 ESP_084814_1205 (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 | -59.2 | 177. | 4.76 | -19.8 | 47.9 | 53.6 |
| Layering in Meridiani Planum Crater: ESP_084161_1810 ESP_084517_1810 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.786 | 356. | 2.30 | -7.87 | 45.2 | 41.8 |
| Fluvially Incised Terrain Northeast of Syrtis Major Planum: ESP_084369_2100 ESP_084514_2100 (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 | 29.56 | 73.9 | -5.8 | 4.318 | 62.3 | 59.8 |
| Dune Change Detection in Mawrth Vallis: ESP_084201_1980 ESP_084135_1980 (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 | 17.79 | 343. | -5.8 | 20.45 | 55.9 | 55.2 |
| Landforms above Subsurface Radar Observations of South Polar Cap: ESP_084325_1000 ESP_084562_1000 (Interval in Earth days: 19) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -80.0 | 222. | -6.3 | 13.65 | 62.6 | 64.0 |
| Possible Volcanic Edifice in Terra Sirenum: ESP_084206_1530 ESP_084562_1530 (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 | -26.8 | 211. | 2.15 | -8.24 | 36.4 | 35.9 |
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