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.
| Arc of Cones with Summit Pits in CTX Image: ESP_019577_1970 ESP_019867_1970 (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 | 16.74 | 198. | -19. | 12.17 | 53.6 | 52.8 |
| 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 |
| 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 |
| 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 |
| Monitoring of Pits and Fractures in Deuteronilus Mensae: ESP_019504_2240 ESP_019570_2240 (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 | 43.81 | 25.2 | 1.42 | -13.1 | 54.7 | 56.8 |
| Ismenius Cavus: ESP_019333_2140 ESP_019478_2140 (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 | 33.77 | 16.9 | -14. | -2.15 | 51.9 | 52.3 |
| 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 |
| Alpine Glacier: ESP_019213_2210 ESP_019503_2210 (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 | 40.86 | 51.3 | -8.0 | 14.46 | 51.2 | 52.7 |
| Gemina Lingula Scarp with Outcrop of Layered Deposits and Unconformities: ESP_018844_2605 ESP_019081_2605 (Interval in Earth days: 19) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 80.37 | 27.0 | 1.70 | 16.54 | 62.6 | 64.5 |
| Steep North Polar Boundary Scarp: ESP_018928_2640 ESP_019034_2640 (Interval in Earth days: 8) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 83.79 | 237. | 7.24 | -7.09 | 65.4 | 67.3 |
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