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.
| Possible Preserved Impact Melt Flow on the Ejecta of Bakhuysen Crater: ESP_031201_1555 ESP_031056_1555 (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 | -24.3 | 13.8 | 17.1 | 1.41 | 33.5 | 36.1 |
| Northern Hellas Planitia Layered Bedrock: ESP_031120_1505 ESP_031898_1505 (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 | -28.9 | 67.3 | 0 | -13.4 | 35.4 | 34.8 |
| Margin of Pedestal Crater in Malea Planum: ESP_030936_1125 ESP_031160_1125 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -67.2 | 61.8 | -15. | 7.116 | 51.8 | 50.4 |
| Light-Toned Stratified Materials in Melas Chasma: ESP_031125_1670 ESP_031903_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 | -13.0 | 289. | -4.6 | -18.9 | 38.4 | 33.6 |
| USGS Dune Database Entry Number 2226-767: ESP_031260_1030 ESP_031062_1030 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -76.6 | 223. | -13. | 3.747 | 58.8 | 57.0 |
| Contact between Wallrock and Light-Toned Layering in Melas Chasma: ESP_031191_1695 ESP_014062_1695 (Interval in Earth days: 1334) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -10.2 | 284. | 23.5 | 4.087 | 36.6 | 35.0 |
| Monitor Seasonal Changes at South Polar Cracked and Gullied Site: ESP_031213_0980 ESP_031266_0980 (Interval in Earth days: 4) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -81.6 | 66.2 | 6.48 | -6.79 | 61.2 | 62.4 |
| Ancient Rocks of the Isidis Basin: PSP_002756_1830 PSP_002822_1830 (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 | 3.174 | 84.9 | 2.98 | -19.6 | 55.7 | 57.7 |
| A Sinuous Ridge in Gale Crater: ESP_030814_1750 ESP_030748_1750 (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 | -4.72 | 138. | 4.50 | 28.32 | 44.8 | 43.7 |
| Alcoves on South Polar Layered Deposit Scarp: ESP_030854_1080 ESP_031078_1080 (Interval in Earth days: 18) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -71.9 | 144. | -17. | -0.98 | 55.2 | 53.9 |
Page 532 of 896 (8,955 images) | |||||