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.
| Aram Chaos: ESP_016750_1830 ESP_017172_1830 (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 | 2.769 | 339. | 3.01 | -13.3 | 47.2 | 51.0 |
| Small Crater Exposed in Cross-Section by Erosion: ESP_016699_1715 ESP_019178_1715 (Interval in Earth days: 193) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.45 | 293. | 1.41 | -13.7 | 52.9 | 58.8 |
| Possible Phyllosilicates in Her Desher Vallis: ESP_016527_1550 ESP_025032_1550 (Interval in Earth days: 663) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -24.8 | 311. | -6.8 | 7.004 | 62.1 | 56.3 |
| Unnamed Crater in Polygonal Terrain in Western Utopia Planitia: ESP_016469_2260 ESP_016535_2260 (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 | 45.59 | 84.3 | 8.50 | -5.58 | 43.4 | 44.2 |
| Layered Deposits along Floor of Melas Chasma: ESP_016673_1700 ESP_017952_1700 (Interval in Earth days: 100) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.67 | 284. | -5.2 | 5.092 | 53.8 | 59.7 |
| Aram Chaos Mineralogical Variability: ESP_016605_1830 ESP_086812_1830 (Interval in Earth days: 5470) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.889 | 339. | -8.3 | -23.3 | 46.9 | 47.0 |
| Contact Between Different Lava Types on Olympus Mons: ESP_016820_1950 ESP_017888_1950 (Interval in Earth days: 83) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 14.85 | 227. | -1.4 | 13.61 | 43.2 | 45.7 |
| Outcrop of Rhythmic Bedding in Arabia Terra: ESP_016657_1890 ESP_017013_1890 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.820 | 358. | -1.3 | 8.534 | 44.4 | 45.7 |
| Light-Toned Layering in Hebes Mensa: ESP_016462_1785 ESP_016818_1785 (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 | -1.35 | 282. | 0.48 | 14.17 | 47.0 | 49.0 |
| Fresh Crater on Alba Patera: ESP_016371_2235 ESP_016226_2235 (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 | 43.05 | 240. | 4.58 | -7.09 | 43.2 | 44.8 |
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