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.
| Exposure of North Polar Layered Deposits: ESP_035568_2655 ESP_036306_2655 (Interval in Earth days: 57) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 85.31 | 268. | -3.7 | 5.673 | 60.5 | 64.0 |
| Faulted Layered Deposits in West Candor Chasma: ESP_035582_1745 ESP_036070_1745 (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 | -5.66 | 283. | -3.0 | -27.7 | 58.0 | 60.2 |
| Impact Monitoring Site in Phlegra Montes: ESP_035362_2190 ESP_060984_2190 (Interval in Earth days: 1997) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 38.72 | 163. | -3.3 | -21.8 | 42.2 | 41.7 |
| Candidate Landing Site for 2020 Mission: ESP_035304_1950 ESP_036148_1950 (Interval in Earth days: 66) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 14.70 | 309. | 8.61 | -3.59 | 45.9 | 49.1 |
| Xanthe Terra Region: ESP_035528_1920 ESP_036873_1920 (Interval in Earth days: 105) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 11.66 | 315. | 0.16 | 11.08 | 48.5 | 51.2 |
| Crater with Steep Slopes: ESP_035246_2105 ESP_035879_2105 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 30.23 | 91.0 | 6.44 | -5.33 | 41.5 | 44.5 |
| Light-Toned Deposits along Coprates Chasma Wallrock Slopes: ESP_035199_1655 ESP_035555_1655 (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 | -14.1 | 300. | -5.2 | 4.733 | 62.5 | 62.8 |
| Young 10-Kilometer Diameter Crater: ESP_035075_2010 ESP_035365_2010 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 20.77 | 82.2 | -6.8 | 20.14 | 44.2 | 42.9 |
| Gully in Crater Wall in Acidalia Planitia: ESP_035118_2330 ESP_035408_2330 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 52.71 | 344. | -8.1 | 8.764 | 44.5 | 43.3 |
| Aram Chaos: ESP_034947_1830 ESP_036503_1830 (Interval in Earth days: 121) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.803 | 338. | 2.06 | 16.03 | 50.6 | 52.8 |
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