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.
| Possible Landing Site for InSight Mission: ESP_042537_1845 ESP_042827_1845 (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 | 4.215 | 135. | -7.8 | 18.80 | 41.7 | 41.7 |
| Contact between Light-Toned Deposits and Wallrock in Northern Melas Chasma: ESP_042492_1720 ESP_045947_1720 (Interval in Earth days: 269) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.94 | 284. | 7.26 | -4.30 | 45.0 | 53.5 |
| Knob near Orcus Patera: ESP_042641_1900 ESP_043142_1900 (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 | 10.11 | 174. | 3.69 | 21.92 | 39.9 | 41.0 |
| Hellespontus Region Dunes: ESP_042290_1380 ESP_042224_1380 (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 | -41.5 | 45.5 | -5.7 | 14.32 | 64.2 | 62.1 |
| Slope Streak in Noctis Labyrinthus: ESP_042651_1745 ESP_043073_1745 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.44 | 263. | 2.15 | -17.0 | 45.7 | 50.7 |
| Overlapping Curved Ridges in Crater in CTX Image: ESP_042567_1510 ESP_042633_1510 (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 | -28.5 | 39.8 | 2.71 | -19.4 | 58.5 | 60.6 |
| Candidate Landing Site for 2020 Mission: ESP_042509_1515 ESP_042008_1515 (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 | -28.4 | 181. | 24.3 | 11.40 | 56.2 | 49.9 |
| Wrinkle Ridges Near Ganges Catena: ESP_042650_1770 ESP_045182_1770 (Interval in Earth days: 198) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.08 | 290. | -0.3 | -23.7 | 44.8 | 54.1 |
| Lobe Partly Covered by Darker Material: ESP_042030_1670 ESP_042531_1670 (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 | -12.9 | 299. | 8.61 | 22.75 | 42.0 | 46.9 |
| Mountain Peak in Charitum Montes: ESP_042452_1290 ESP_033485_1290 (Interval in Earth days: 699) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -50.7 | 301. | 16.6 | -1.15 | 72.2 | 70.6 |
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