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.
| Alluvial Fans in Kasei Valles: ESP_085574_2030 ESP_085640_2030 (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 | 22.67 | 293. | 15.8 | 1.691 | 42.0 | 42.6 |
| Layered Deposits in Melas Chasma: ESP_085535_1695 ESP_085746_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 | -10.1 | 284. | -7.5 | 8.858 | 37.4 | 38.0 |
| Head of Lethe Vallis: ESP_085698_1840 ESP_086265_1840 (Interval in Earth days: 45) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.812 | 153. | -1.1 | -19.3 | 37.1 | 41.8 |
| Crater in Acidalia Planitia: ESP_085692_2225 ESP_085349_2225 (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 | 42.12 | 312. | 0.45 | 14.56 | 53.6 | 57.1 |
| Flow Ridge in Nereidum Montes: ESP_085587_1340 ESP_085732_1340 (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 | -45.6 | 310. | -6.8 | 16.93 | 55.1 | 56.2 |
| Small Volcanic Cones in Chryse Chaos: ESP_085362_1885 ESP_085573_1885 (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 | 8.322 | 324. | -6.6 | 4.325 | 38.7 | 37.3 |
| Stepped Features in Tartarus Skopulus: ESP_085684_1800 ESP_085829_1800 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.074 | 175. | 2.52 | 26.97 | 36.6 | 35.2 |
| Glacier-Like Form Terminus into Valley Fill: ESP_085405_2185 ESP_085748_2185 (Interval in Earth days: 26) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 37.97 | 226. | -4.2 | -17.4 | 54.5 | 51.5 |
| Inverted Channel Noachis Terra: ESP_085387_1505 ESP_085598_1505 (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 | -29.1 | 5.42 | 6.72 | 17.19 | 41.3 | 43.5 |
| Large Isolated Landform at Chryse Planitia Margin: ESP_085402_1945 ESP_085547_1945 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 14.22 | 310. | 5.37 | 29.46 | 39.9 | 37.2 |
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