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.
Mojave Crater Southern Rim - Putative Melt-Bearing Flows: PSP_007995_1875 PSP_009432_1875 (Interval in Earth days: 112) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.168 | 327. | -3.2 | 15.34 | 46.7 | 50.9 |
Topographically-Deflected Ejecta in Chryse Planitia: PSP_007916_2010 ESP_016078_2010 (Interval in Earth days: 636) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 20.91 | 322. | 0.50 | 15.41 | 41.8 | 38.0 |
Small Lava Flows Emanating From the Cerberus Fossae: PSP_007197_1910 PSP_008199_1910 (Interval in Earth days: 78) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 10.63 | 156. | 5.84 | -4.05 | 39.2 | 46.5 |
Area Near Summit of Gale Crater Mound: PSP_008002_1750 PSP_009927_1750 (Interval in Earth days: 151) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.85 | 137. | -5.8 | -22.8 | 52.8 | 59.9 |
Central Peak of Unnamed Crater within the Medusae Fossae Formation: PSP_007870_1830 PSP_009228_1830 (Interval in Earth days: 106) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.031 | 140. | 4.36 | -20.5 | 47.0 | 55.2 |
Chasma Borealis: PSP_007020_2580 PSP_007178_2580 (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 | 77.78 | 292. | 0 | 12.81 | 69.8 | 67.1 |
Central Peak and Floor of Large Crater West of Schiaparelli Crater: PSP_007822_1775 PSP_008178_1775 (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 | -2.30 | 11.7 | 2.98 | -8.20 | 49.3 | 52.9 |
Stair-Stepped Slope Seen in MOC Image R08-00823: PSP_007684_1795 ESP_020171_1795 (Interval in Earth days: 973) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.44 | 180. | -5.7 | 17.22 | 47.7 | 53.5 |
Slope Streaks Beginning at Stratigraphic Layers: PSP_007473_1850 PSP_008264_1850 (Interval in Earth days: 62) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.996 | 181. | -5.4 | 5.46 | 43.6 | 48.7 |
Light-Toned Tilted Layering in Central Peak of Oudemans Crater: PSP_007694_1700 ESP_027882_1700 (Interval in Earth days: 1574) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.92 | 268. | 1.09 | -17.4 | 52.3 | 59.3 |
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