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.
| 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 |
| Layering in Yorktown Crater: ESP_020865_2030 ESP_065330_2030 (Interval in Earth days: 3465) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 22.90 | 311. | 2.61 | 22.55 | 62.8 | 65.6 |
| 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 |
| Channels and Lava Flows: ESP_020261_2010 ESP_020683_2010 (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 | 20.66 | 241. | 6.17 | -9.72 | 57.1 | 61.6 |
| Bedrock Layers Exposed in West Proctor Crater: ESP_020256_1320 ESP_020889_1320 (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 | -47.6 | 28.2 | -5.3 | -20.9 | 67.7 | 58.9 |
| Spiders in Variety of Terrains: ESP_020229_0930 ESP_020230_0930 (Interval in Earth days: 0) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.0 | 86.4 | 9.23 | -2.36 | 88.6 | 89.9 |
| Sinuous Ridges in Aeolis and Zephyria Regions: ESP_020383_1740 ESP_020805_1740 (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 | -6.00 | 153. | 12.3 | -2.66 | 53.9 | 53.9 |
| Sinuous Ridges in Crater near Reull Vallis: ESP_020055_1410 ESP_020121_1410 (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 | -38.4 | 113. | 8.56 | -9.74 | 65.3 | 65.8 |
| Massif on the Floor of Coprates Chasma: ESP_020246_1680 ESP_020958_1680 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.1 | 296. | -6.3 | 10.26 | 56.4 | 51.3 |
Page 654 of 900 (8,995 images) | |||||