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.
| Small But Very Deep Pit North of Arsia Mons: PSP_007774_1745 PSP_008130_1745 (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 | -5.30 | 242. | 6.40 | -5.72 | 50.2 | 54.0 |
| Western Portion and Ejecta of Well-Preserved Crater: PSP_007804_1970 PSP_009307_1970 (Interval in Earth days: 117) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 16.91 | 141. | -5.6 | -18.2 | 42.5 | 49.1 |
| Ring and Cone Structures in Grjota Valles: PSP_007869_1960 PSP_007579_1960 (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 | 15.90 | 164. | 18.0 | 4.908 | 41.1 | 40.7 |
| Olympus Mons North Scarp Detail: PSP_007735_2030 PSP_008091_2030 (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 | 22.92 | 224. | 4.41 | -5.92 | 40.5 | 42.5 |
| Diverse Features in Utopia Region: PSP_007951_2220 PSP_008162_2220 (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 | 41.58 | 82.8 | 6.93 | -5.86 | 41.7 | 42.5 |
| Light-Toned Layering in Melas Chasma: PSP_007812_1700 PSP_010660_1700 (Interval in Earth days: 222) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.87 | 285. | 5.77 | -12.6 | 53.1 | 60.5 |
| Preserved Fans in Unnamed Crater in Tartarus Region: PSP_008093_1995 PSP_008383_1995 (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 | 19.47 | 169. | -4.6 | 6.092 | 43.2 | 43.4 |
| Faulted Layers in Impact Crater: PSP_008023_1745 PSP_010238_1745 (Interval in Earth days: 173) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.29 | 284. | -3.7 | 13.99 | 53.0 | 57.2 |
| Small Crater with Layered Fill in Schiaparelli Crater: PSP_007400_1790 PSP_007756_1790 (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 | -0.75 | 14.3 | 9.35 | -3.82 | 44.1 | 48.4 |
| Possible Sulfates in Coprates Chasma: PSP_007205_1660 ESP_024505_1660 (Interval in Earth days: 1348) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.9 | 301. | 5.58 | -16.3 | 48.4 | 44.1 |
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