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.
| Crater Fill Deposit: ESP_020532_1465 ESP_020677_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 | -33.1 | 50.6 | -7.0 | 7.211 | 58.6 | 55.7 |
| Material Flowing Through Gap in Crater Rim East of Hellas Planitia: ESP_020543_1345 ESP_029246_1345 (Interval in Earth days: 678) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -45.2 | 111. | -0.3 | 25.69 | 62.1 | 61.5 |
| Layered Terrain between Aeolis and Zephyria Plana: ESP_020594_1735 ESP_020739_1735 (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 | -6.38 | 153. | -1.7 | 14.49 | 54.5 | 52.8 |
| Ejecta of Very Well-Preserved Crater: ESP_020723_2235 ESP_064845_2235 (Interval in Earth days: 3438) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 43.26 | 225. | -4.6 | 28.28 | 72.1 | 71.8 |
| Circular Features in Western Elysium Planitia: ESP_020911_1850 ESP_021623_1850 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.702 | 138. | -7.0 | 3.973 | 56.5 | 53.1 |
| Slope Streaks on Wall of Nicholson Crater: ESP_020421_1810 ESP_081543_1810 (Interval in Earth days: 4763) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 1.037 | 195. | 7.05 | -1.74 | 54.6 | 57.9 |
| Bedrock Exposure in Landslide Scarp: ESP_020879_1670 ESP_021657_1670 (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 | -12.9 | 293. | 5.19 | -7.68 | 52.2 | 46.1 |
| Sinuous Ridges in the Aeolis/Zephyria Region: ESP_020528_1750 ESP_020673_1750 (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 | -5.06 | 154. | 7.87 | 22.67 | 54.0 | 52.4 |
| Fan and Valley within Crater: ESP_020323_2050 ESP_020824_2050 (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 | 24.54 | 348. | -1.3 | 18.52 | 59.4 | 62.1 |
| Fresh 8-Kilometer Diameter Impact Crater near Vistula Valles: ESP_020219_1940 ESP_020852_1940 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 13.75 | 308. | 8.31 | -14.0 | 55.3 | 60.2 |
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