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.
| Valleys in Crater Northeast of Argyre Planitia: ESP_064736_1500 ESP_064591_1500 (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 | -29.7 | 335. | 0.30 | -16.8 | 58.2 | 61.0 |
| Floor of East Candor Chasma: ESP_064843_1730 ESP_064487_1730 (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 | -6.89 | 291. | -8.7 | -23.9 | 57.4 | 59.4 |
| Blocky Terrain in Elysium Planitia: ESP_064835_1830 ESP_090432_1830 (Interval in Earth days: 1994) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.193 | 147. | 5.27 | -16.6 | 58.1 | 57.9 |
| Landforms in Utopia Planitia: ESP_064796_2010 ESP_065284_2010 (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 | 20.69 | 132. | -18. | -29.2 | 65.0 | 68.3 |
| Network of Sinuous Ridges in Aeolis Dorsa: ESP_064848_1730 ESP_073039_1730 (Interval in Earth days: 638) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.70 | 154. | 4.51 | -24.5 | 56.4 | 60.0 |
| Valleys in Central Pit of Crater: ESP_064630_1525 ESP_073599_1525 (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 | -27.4 | 347. | 8.33 | -13.2 | 58.2 | 58.2 |
| Gully Monitoring: ESP_064726_1390 ESP_065491_1390 (Interval in Earth days: 60) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -40.8 | 249. | -0.4 | -21.8 | 61.0 | 52.1 |
| 4-Kilometer Rayed Crater: ESP_064513_1870 ESP_074260_1870 (Interval in Earth days: 759) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 6.696 | 298. | 3.19 | -7.81 | 58.0 | 58.9 |
| Light-Toned Knobby Unit in Degraded Crater: ESP_064772_1715 ESP_065260_1715 (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 | -8.40 | 69.9 | -4.7 | -20.2 | 57.2 | 56.3 |
| Transition from Channel to Ridge: ESP_064841_1565 ESP_065751_1565 (Interval in Earth days: 71) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -23.4 | 348. | -6.5 | 5.135 | 56.9 | 46.6 |
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