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.
| Small Volcano in Wind Streak Southwest of Tombaugh Crater: ESP_035204_1830 ESP_035270_1830 (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 | 2.862 | 160. | 11.9 | -11.2 | 51.0 | 52.9 |
| Domoni Crater Secondaries: ESP_035056_2310 ESP_035188_2310 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 50.65 | 235. | -0.7 | -25.8 | 43.2 | 45.6 |
| Pits in Sinai Planum: ESP_035266_1710 ESP_035411_1710 (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 | -8.95 | 271. | -5.1 | 11.84 | 59.3 | 58.7 |
| Meridiani Planum: ESP_034986_1785 ESP_042806_1785 (Interval in Earth days: 609) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.70 | 353. | 8.72 | -26.4 | 52.9 | 47.6 |
| Flow Feature West of Meridiani Planum: ESP_034973_1780 ESP_035118_1780 (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 | -1.95 | 349. | -5.9 | 8.914 | 53.9 | 53.6 |
| Athabasca Valles Distributary Channel: ESP_035191_1880 ESP_036457_1880 (Interval in Earth days: 99) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.051 | 155. | 6.56 | -7.04 | 48.6 | 52.4 |
| Candidate Landing Site for 2020 Mission: ESP_035263_1795 ESP_036964_1795 (Interval in Earth days: 132) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.36 | 351. | -1.1 | 17.84 | 53.9 | 54.2 |
| Outflow Channel Features Associated with Small Chaotic Terrain: ESP_035067_1775 ESP_036544_1775 (Interval in Earth days: 116) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.50 | 302. | 2.75 | -21.9 | 54.1 | 58.1 |
| Candidate Future Landing Site: ESP_034907_1825 ESP_034841_1825 (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 | 2.529 | 351. | -3.8 | 19.79 | 51.0 | 48.9 |
| Outflow Channel Features in Arena Colles: ESP_035220_2085 ESP_036486_2085 (Interval in Earth days: 99) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 28.23 | 81.1 | 7.68 | -4.51 | 41.7 | 47.8 |
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