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.
Central Uplift of an Impact Crater: ESP_017603_1550 ESP_026095_1550 (Interval in Earth days: 661) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -24.7 | 94.5 | 2.99 | -24.4 | 69.4 | 68.6 |
Central Uplift of an Impact Crater: ESP_017434_1525 ESP_027139_1525 (Interval in Earth days: 757) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.0 | 29.6 | -4.8 | 16.90 | 70.8 | 69.6 |
Nili Patera Caldera and Dunes: ESP_017617_1890 ESP_034891_1890 (Interval in Earth days: 1346) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.020 | 67.5 | 9.95 | -9.19 | 47.9 | 48.1 |
Valley along Noctis Labrynthus Floor: ESP_017465_1730 ESP_017966_1730 (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 | -7.16 | 261. | -10. | 10.24 | 57.8 | 57.8 |
Well-Preserved 1-Kilometer Diameter Impact Crater on Northern Plains: ESP_017480_2355 ESP_017968_2355 (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 | 55.21 | 200. | 6.86 | -14.0 | 44.1 | 46.3 |
Channels and Streamlined Landforms: ESP_017666_1935 ESP_017732_1935 (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 | 13.13 | 169. | 9.37 | -13.0 | 46.2 | 48.1 |
Layered Deposits in Candor Chasma: ESP_017675_1760 ESP_017886_1760 (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 | -4.13 | 285. | 5.36 | -4.03 | 55.6 | 56.7 |
Crater Next to Crater with Dark Gully Deposits: ESP_017312_1465 ESP_053825_1465 (Interval in Earth days: 2845) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -33.3 | 121. | -6.5 | -17.0 | 74.9 | 74.3 |
Cone with Lobate Flows in Hydraotes Chaos: ESP_017634_1800 ESP_025493_1800 (Interval in Earth days: 612) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.10 | 326. | -12. | -26.9 | 54.3 | 49.1 |
Southern Gale Crater Strata with Possible Sulfates and Clays: ESP_017364_1745 ESP_017509_1745 (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 | -5.59 | 138. | -8.2 | 6.376 | 56.3 | 55.9 |
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