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.
| InSight Mission Candidate Landing Site: ESP_037829_1840 ESP_038383_1840 (Interval in Earth days: 43) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.983 | 137. | 10.4 | -4.64 | 55.9 | 58.2 |
| Meridiani Planum Stratigraphy: ESP_037847_1805 ESP_038401_1805 (Interval in Earth days: 43) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.330 | 6.52 | 9.92 | -3.02 | 56.0 | 57.3 |
| Channelized Flow in Arimanes Rupes Region East of Mangala Valles: ESP_037734_1675 ESP_046754_1675 (Interval in Earth days: 703) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.2 | 213. | 1.74 | -10.3 | 58.0 | 53.1 |
| Alluvial Fans in Crater: ESP_037730_1615 ESP_038007_1615 (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 | -18.4 | 322. | 6.49 | -10.4 | 59.1 | 58.8 |
| Boulders inside of Pits on a Mesa: ESP_037747_1810 ESP_073986_1810 (Interval in Earth days: 2824) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 1.014 | 217. | -6.3 | 20.01 | 57.1 | 55.5 |
| Bright and Dark Fans in Region Dubbed Manhattan: ESP_037976_0940 ESP_037977_0940 (Interval in Earth days: 0) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -85.6 | 105. | 22.2 | -1.02 | 84.6 | 86.6 |
| Inverted Channels on Valley Floor: ESP_037612_1400 ESP_045999_1400 (Interval in Earth days: 653) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.6 | 307. | -2.6 | 9.005 | 68.6 | 68.8 |
| Crater in Tempe Terra: ESP_037691_2170 ESP_045999_2170 (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 | 36.64 | 299. | 13.0 | -7.66 | 60.2 | 51.0 |
| Monitoring Wind Streak and Intracrater Dunes: ESP_037603_1920 ESP_037669_1920 (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 | 11.80 | 185. | 8.55 | -11.1 | 55.1 | 57.2 |
| Crater Floor: ESP_037851_1780 ESP_038405_1780 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.92 | 257. | 12.7 | -0.09 | 55.8 | 56.6 |
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