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.
| Resistant Layer in Medusae Fossae Formation: ESP_082729_1830 ESP_083230_1830 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.727 | 217. | -6.6 | 0.505 | 58.9 | 56.0 |
| Intracrater Landslide South of Pyrrhae Chaos: ESP_082646_1485 ESP_082936_1485 (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 | -31.3 | 328. | -2.5 | 8.715 | 55.7 | 51.0 |
| Channel in Rahway Valles: ESP_082612_1895 ESP_082190_1895 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.640 | 173. | -27. | -8.00 | 63.1 | 60.4 |
| Small Flow Channels: ESP_082842_1480 ESP_083132_1480 (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 | -31.6 | 15.7 | 0.54 | 20.15 | 52.9 | 47.3 |
| Small Group of Dark Dunes in Aurorae Chaos: ESP_082514_1725 ESP_082725_1725 (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 | -7.47 | 330. | -1.2 | -26.7 | 57.0 | 58.0 |
| Jarosite-Rich Terrain in Northern Nili Fossae: ESP_082800_2075 ESP_082879_2075 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 27.03 | 74.9 | 3.37 | 29.71 | 68.6 | 66.9 |
| Graben-Crater Intersection at Tantalus Fossae: ESP_082648_2260 ESP_082727_2260 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 45.90 | 262. | 7.49 | 26.08 | 77.2 | 76.6 |
| Small Delta or Fan: ESP_082815_1490 ESP_083105_1490 (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 | -30.5 | 32.7 | 3.11 | 21.53 | 53.0 | 47.6 |
| Transect Across Lower Harmakhis Vallis: ESP_082813_1370 ESP_074413_1370 (Interval in Earth days: 655) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -42.6 | 86.3 | 27.1 | 4.948 | 52.8 | 48.0 |
| Outcrop in Athabasca Valles Lava: ESP_082705_1880 ESP_082270_1880 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.779 | 149. | 27.6 | 7.677 | 57.8 | 59.0 |
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