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.
| Dune Monitoring in Crater: ESP_081463_2450 ESP_090258_2450 (Interval in Earth days: 686) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 64.85 | 209. | -2.0 | -15.7 | 68.5 | 68.8 |
| Streamlined Landforms adjacent to Shalbatana Vallis: ESP_081512_1890 ESP_080800_1890 (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 | 8.966 | 318. | 28.8 | 14.43 | 54.2 | 53.2 |
| Southern Canyon Wall in East Coprates Chasma: ESP_081605_1640 ESP_081671_1640 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.6 | 304. | 7.52 | -13.4 | 60.9 | 62.2 |
| Faulted Concentric Crater Fill Northeast of Elysium Region: ESP_081531_2155 ESP_081452_2155 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.03 | 157. | 9.04 | -21.0 | 58.3 | 59.9 |
| Small Gullies on Ridge and Lobate Flows on Crater Floor: ESP_081539_1360 ESP_081882_1360 (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 | -43.7 | 309. | 13.8 | -16.5 | 72.5 | 70.3 |
| Possible Future Landing Site in Utopia Region: ESP_081466_1835 ESP_081611_1835 (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 | 3.614 | 136. | 8.62 | 26.26 | 56.5 | 55.3 |
| Exposed Portions of Uplift in 30-Km Crater in Terra Sabaea: ESP_081693_1605 ESP_081759_1605 (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 | -19.1 | 63.9 | -10. | -28.3 | 62.9 | 64.0 |
| Lobate Feature in Post-Glacial Region: ESP_081566_2060 ESP_081843_2060 (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 | 25.48 | 284. | -2.5 | -18.9 | 57.9 | 62.0 |
| Isolated Dunes and Sand Patches Southeast of Syrtis Major: ESP_081600_1980 ESP_089986_1980 (Interval in Earth days: 654) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.60 | 78.4 | -13. | 8.609 | 58.3 | 52.4 |
| Well-Exposed Massif with Diverse Bedrock Exposures North of Hellas Region: ESP_081574_1565 ESP_081917_1565 (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 | -23.5 | 71.7 | 6.18 | -28.8 | 63.9 | 64.1 |
Page 100 of 896 (8,955 images) | |||||