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.
| Gullies and Possible Flow Features: ESP_025177_1525 ESP_025744_1525 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.1 | 314. | -7.7 | 4.178 | 60.6 | 66.0 |
| Fine-Scale Reticulate Bedform Change Detection in Daedalia Planum: ESP_025391_1750 ESP_025101_1750 (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 | -5.09 | 226. | 27.6 | -5.91 | 46.7 | 46.1 |
| Fresh Crater on Northern Plains: ESP_025116_2320 ESP_025195_2320 (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 | 51.71 | 172. | -20. | 0.151 | 48.6 | 46.4 |
| Light-Toned Layering along Plains South of Melas Region: ESP_025310_1690 ESP_025455_1690 (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 | -10.8 | 281. | -9.0 | 9.973 | 51.7 | 52.0 |
| Peridier Crater Dune Changes: ESP_025383_2055 ESP_025528_2055 (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 | 25.09 | 83.5 | 2.17 | 17.79 | 38.8 | 37.8 |
| Kipuka in Amazonis Planitia: ESP_025181_1950 ESP_025669_1950 (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 | 14.70 | 200. | -3.0 | -27.5 | 39.6 | 44.4 |
| Fresh Small Rayed Crater: ESP_025174_1660 ESP_028207_1660 (Interval in Earth days: 236) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.0 | 34.6 | -2.7 | 6.91 | 51.7 | 58.6 |
| Strange Features in Hellas Basin: ESP_025160_1445 ESP_042395_1445 (Interval in Earth days: 1343) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -35.2 | 58.5 | 10.2 | -13.7 | 65.2 | 61.7 |
| Stratified Material in Pit as Seen in CTX Image : ESP_025259_1825 ESP_026881_1825 (Interval in Earth days: 127) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.450 | 231. | 6.43 | -8.79 | 43.3 | 52.6 |
| Impact Crater with Central Pit on Floor of Larger Crater: ESP_025240_1690 ESP_025728_1690 (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 | -10.6 | 31.9 | 2.87 | -23.9 | 50.1 | 56.6 |
Page 609 of 900 (8,995 images) | |||||