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.
| Features in Echus Chasma: ESP_068049_1805 ESP_072665_1805 (Interval in Earth days: 360) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.707 | 279. | 4.52 | 27.80 | 41.1 | 54.4 |
| Mesa with Bright Spot in Oxia Colles: ESP_067849_2055 ESP_068245_2055 (Interval in Earth days: 31) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 25.41 | 333. | -12. | -24.5 | 49.3 | 48.5 |
| Cross-Cutting Faults Southeast of Melas Chasma: ESP_067732_1650 ESP_073746_1650 (Interval in Earth days: 468) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.9 | 290. | -14. | 16.69 | 41.5 | 54.0 |
| Troughs and Ridges in Chryse Planitia: ESP_067823_2105 ESP_067480_2105 (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 | 30.33 | 319. | 13.9 | -5.70 | 50.2 | 54.9 |
| Collapse Terrain near Orson Welles Crater: ESP_068061_1785 ESP_072677_1785 (Interval in Earth days: 360) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.50 | 313. | 1.23 | 21.77 | 41.5 | 55.4 |
| Crater Floor Outcrop: ESP_067980_2160 ESP_063970_2160 (Interval in Earth days: 312) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.60 | 0.43 | -22. | -12.2 | 54.5 | 59.7 |
| Very Fresh Small Impact Crater: ESP_067714_1815 ESP_076827_1815 (Interval in Earth days: 710) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 1.484 | 59.1 | -5.1 | 8.893 | 40.7 | 36.3 |
| Inverted Channel in Cusus Valles: ESP_067833_1960 ESP_067965_1960 (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 | 16.05 | 49.8 | 5.88 | -3.77 | 43.8 | 44.2 |
| Two Notches near Lowest Elevation Point of Crater Rim: ESP_067821_1465 ESP_067689_1465 (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 | -33.2 | 24.7 | -7.3 | 6.887 | 48.4 | 45.5 |
| Valleys in Crater Northeast of Argyre Region: ESP_067704_1500 ESP_073784_1500 (Interval in Earth days: 474) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -29.6 | 334. | 7.13 | 20.86 | 44.0 | 53.7 |
Page 196 of 891 (8,901 images) | |||||