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.
| North Polar Layered Deposits 160-Meter Diameter Crater Monitoring : ESP_044810_2620 ESP_044784_2620 (Interval in Earth days: 2) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 81.84 | 333. | 7.95 | -6.74 | 59.0 | 59.6 |
| Meridiani Planum : ESP_044718_1780 ESP_046274_1780 (Interval in Earth days: 122) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.19 | 354. | 2.37 | 19.53 | 52.6 | 49.7 |
| Unusual Crater in Amazonis Planitia : ESP_044855_2090 ESP_044921_2090 (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 | 28.72 | 210. | 3.03 | -12.8 | 41.0 | 42.5 |
| North Polar Layered Deposits Exposure: ESP_044982_2670 ESP_044706_2670 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 87.05 | 306. | -8.9 | -21.3 | 64.7 | 63.6 |
| Exposure of North Polar Layered Deposits : ESP_044495_2695 ESP_044718_2695 (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 | 89.44 | 3.84 | -28. | -26.0 | 65.2 | 65.7 |
| Eos Chasma : ESP_044403_1625 ESP_052051_1625 (Interval in Earth days: 596) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -17.0 | 315. | -6.0 | -25.3 | 62.9 | 58.5 |
| Channel Forms in Plain in CTX Image: ESP_044279_1465 ESP_052573_1465 (Interval in Earth days: 647) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -33.2 | 102. | -4.9 | 7.263 | 74.5 | 72.2 |
| Valley in Crater : ESP_044330_1685 ESP_070099_1685 (Interval in Earth days: 2008) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.2 | 146. | 6.71 | -10.9 | 58.2 | 65.3 |
| Western Rim and Ejecta of Fresh 8-Kilometer Crater in Margaritifer Terra : ESP_044349_1605 ESP_043861_1605 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -19.2 | 348. | 6.98 | 27.09 | 63.7 | 61.6 |
| Highland to Lowland Transition in Deuteronilus Region : ESP_044493_2255 ESP_045627_2255 (Interval in Earth days: 88) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 45.31 | 10.4 | -3.9 | 26.46 | 41.2 | 45.9 |
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