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.
| Channels and Vents in Tharsis Region: ESP_019483_2010 ESP_019549_2010 (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 | 20.54 | 241. | 2.59 | -17.9 | 50.9 | 53.1 |
| Decameter-Scale Patterned Ground and Possible Pits: ESP_019551_2010 ESP_020263_2010 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.00 | 186. | -14. | 6.714 | 52.9 | 57.2 |
| Exposure of North Polar Layered Deposits: ESP_019283_2675 ESP_018978_2675 (Interval in Earth days: 24) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 87.36 | 264. | -12. | 0 | 73.2 | 69.5 |
| Rayed Crater in Arcadia Region in Themis V35985012: ESP_019590_2265 ESP_020078_2265 (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 | 46.31 | 197. | -0.0 | -17.7 | 56.8 | 65.6 |
| Western Edge of Hellas Planitia: ESP_019596_1365 ESP_020084_1365 (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 | -43.2 | 44.5 | 8.05 | -14.8 | 73.1 | 68.8 |
| Sinuous Ridges with Scroll Bars at a Scarp: ESP_019328_1750 ESP_019961_1750 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.04 | 155. | 16.6 | 2.067 | 54.9 | 55.3 |
| Fissures in Tempe Terra: ESP_019508_2245 ESP_019574_2245 (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 | 43.91 | 276. | -3.8 | -18.2 | 55.2 | 57.3 |
| Rocky Central Structure of a Large 40-Kilometer Diameter Crater: ESP_019441_1595 ESP_019942_1595 (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 | -20.2 | 314. | -5.7 | 23.31 | 62.9 | 57.7 |
| Diverse Bedrock Exposures on Floor of Nili Patera: ESP_019595_1890 ESP_019740_1890 (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 | 9.085 | 67.0 | -15. | 1.288 | 53.9 | 53.1 |
| Well-Preserved 10-Kilometer Diameter Impact Crater: ESP_019561_1980 ESP_019917_1980 (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 | 17.94 | 272. | 6.73 | 18.70 | 51.2 | 52.7 |
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