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.
| Intracrater Dunes Superposed on Ridges on Fan Surface: ESP_024913_1580 ESP_025625_1580 (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 | -21.5 | 320. | 7.35 | 29.03 | 52.5 | 59.4 |
| Scarp around Crater Ejecta as Seen in CTX Image: ESP_024628_1720 ESP_024839_1720 (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 | -7.78 | 179. | 6.80 | -4.63 | 41.1 | 44.4 |
| Intracrater Sand Dunes and Patch Changes: ESP_024838_1630 ESP_024693_1630 (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 | -16.7 | 207. | 0.91 | -12.4 | 48.8 | 47.8 |
| Slope Streak and Reticulate Bedform Monitoring: ESP_024719_2040 ESP_025009_2040 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.79 | 212. | -7.7 | 17.03 | 38.5 | 36.7 |
| Proposed Site for Future Exploration in Ladon Valles: ESP_024728_1595 ESP_024227_1595 (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 | -20.5 | 329. | 21.3 | -1.13 | 48.3 | 42.5 |
| Patch of Rocky Ground: ESP_024922_1570 ESP_034482_1570 (Interval in Earth days: 745) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -22.8 | 75.5 | 0 | 26.21 | 53.9 | 61.8 |
| Small Mounds in Chryse Planitia: ESP_024715_1995 ESP_025638_1995 (Interval in Earth days: 72) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 19.41 | 322. | -11. | 2.369 | 38.2 | 40.4 |
| Sand Dune Changes in Hellespontus Montes: ESP_024686_1340 ESP_024462_1340 (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 | -45.4 | 38.8 | 28.3 | -5.74 | 64.8 | 63.1 |
| Impact Crater: ESP_024621_1760 ESP_025043_1760 (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 | -4.18 | 11.0 | 3.05 | -16.6 | 39.8 | 45.9 |
| Central Peak of Unnamed Crater in Thaumasia Planum Mountains: ESP_024731_1460 ESP_024230_1460 (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 | -33.6 | 252. | -5.2 | -25.1 | 58.7 | 52.0 |
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