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 with Tributaries on Rocky Plains Northwest of Argyre Region: ESP_064645_1320 ESP_082568_1320 (Interval in Earth days: 1397) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -47.5 | 301. | 5.97 | -6.62 | 63.9 | 60.6 |
| Flow Features in Reull Vallis: ESP_064837_1405 ESP_065391_1405 (Interval in Earth days: 43) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.4 | 96.2 | 28.3 | 5.137 | 56.8 | 51.1 |
| Flow Features Associated with Well-Preserved 10-Kilometer Crater: ESP_064722_1605 ESP_065500_1605 (Interval in Earth days: 61) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -19.4 | 356. | -7.7 | 26.05 | 57.6 | 48.3 |
| Crater Floor Bench in Hellas Region Rim Crater: ESP_064864_1505 ESP_055567_1505 (Interval in Earth days: 724) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -28.9 | 83.6 | -29. | -8.79 | 59.3 | 58.1 |
| Distal Extent of Inverted Delta Material: ESP_064631_1925 ESP_072690_1925 (Interval in Earth days: 628) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 12.36 | 315. | 4.63 | 28.07 | 59.6 | 53.1 |
| Circular Landform North of Kasei Valles: ESP_064869_2085 ESP_074972_2085 (Interval in Earth days: 787) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 28.06 | 296. | 2.44 | -23.2 | 66.9 | 68.6 |
| Inverted Channels: ESP_064527_1440 ESP_055573_1440 (Interval in Earth days: 698) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -35.6 | 280. | 9.24 | -8.74 | 61.2 | 60.4 |
| Nicholson Crater: ESP_064530_1800 ESP_064807_1800 (Interval in Earth days: 22) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.058 | 195. | -0.4 | -23.4 | 57.6 | 59.8 |
| Small Barchan Dunes in Northeast Argyre Region: ESP_064789_1350 ESP_064723_1350 (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 | -44.6 | 331. | -5.9 | 10.38 | 61.7 | 61.4 |
| Vent and Fissure System East of Olympus Mons: ESP_064700_1975 ESP_064555_1975 (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 | 17.54 | 233. | -14. | -29.2 | 62.9 | 63.2 |
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