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_085363_2035 ESP_085297_2035 (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 | 23.14 | 294. | 0.51 | 16.99 | 45.1 | 44.7 |
| Northern Terra Cimmeria: ESP_085541_1740 ESP_086319_1740 (Interval in Earth days: 61) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.31 | 119. | 3.84 | -8.46 | 36.1 | 44.2 |
| North Pole Facing Deposit in Crater: ESP_085325_2220 ESP_085813_2220 (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 | 41.70 | 249. | -2.3 | 2.947 | 58.0 | 51.8 |
| 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 |
| Landforms above Subsurface Radar Observations of South Polar Cap: ESP_085526_1000 ESP_085513_1000 (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 | -79.7 | 185. | 8.77 | -3.25 | 79.0 | 79.5 |
| Ridges near Vernal Crater: ESP_085651_1840 ESP_086218_1840 (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 | 3.944 | 356. | 3.12 | -8.10 | 36.7 | 40.5 |
| Incised Gullies: ESP_085346_1395 ESP_085491_1395 (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 | -39.9 | 46.0 | 6.28 | 26.83 | 46.8 | 47.7 |
| Tributary Channel Surrounded by Complex Craters: ESP_085414_2060 ESP_085981_2060 (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 | 25.96 | 341. | 1.97 | 22.76 | 46.2 | 40.5 |
| 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 |
| Landform and Dunes in Arabia Terra: ESP_085625_1910 ESP_085836_1910 (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 | 10.95 | 345. | -6.7 | 2.615 | 38.8 | 38.0 |
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