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.
| Rocky Deposit That Appears to Emanate from Warrego Valles Channel: ESP_012665_1365 ESP_012731_1365 (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 | -43.1 | 268. | 8.21 | -10.4 | 47.9 | 48.3 |
| Candidate Landing Site in Terra Sabaea and Tyrrhenna Terra Boundary: ESP_013925_1580 ESP_014426_1580 (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 | -21.7 | 66.6 | 0.50 | 25.72 | 34.3 | 32.1 |
| Fluvial Channel in Crommelin Crater: ESP_013097_1850 ESP_030582_1850 (Interval in Earth days: 1362) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.948 | 349. | -6.8 | 21.51 | 53.5 | 51.0 |
| Layers in Spallanzani Crater: ESP_013041_1215 ESP_013120_1215 (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 | -58.1 | 86.8 | 5.04 | 26.10 | 48.1 | 45.8 |
| Layering in Crater: ESP_013057_1825 ESP_013769_1825 (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 | 2.613 | 1.41 | 3.63 | 16.95 | 51.9 | 42.7 |
| Possible Olivine-Rich Terrain in Ejecta of a Gullied Crater: ESP_012761_1430 ESP_013117_1430 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -36.8 | 167. | 6.94 | 17.27 | 45.6 | 40.1 |
| Mawrth Region Stratigraphy in Crater Wall: ESP_013651_2045 ESP_014284_2045 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.04 | 342. | -2.1 | -22.0 | 59.6 | 52.4 |
| Bedrock Exposures in Central Uplift of Large Crater North of Eos Chasma: ESP_013151_1685 ESP_013573_1685 (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 | -11.2 | 317. | -0.6 | -17.0 | 44.8 | 40.9 |
| Ridges at the Edge of the Layered Deposits within Reynolds Crater: ESP_013169_1055 ESP_013301_1055 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -74.2 | 200. | -3.6 | -17.2 | 56.4 | 57.0 |
| Layered Alunite-Kaolinite Deposit: ESP_013775_1490 ESP_021924_1490 (Interval in Earth days: 635) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -30.4 | 202. | 4.83 | 29.52 | 34.9 | 36.8 |
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