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.
| Odd Layered and Eroding Crater Fill in Deeply Eroded Craters: PSP_003773_1630 PSP_003918_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 | -16.8 | 42.7 | 1.82 | 18.06 | 48.1 | 45.3 |
| Light-Toned Layering in Ius Chasma: PSP_003593_1725 ESP_058000_1725 (Interval in Earth days: 4239) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.48 | 275. | 4.77 | -11.1 | 51.7 | 34.5 |
| Dark Materials on Block in Olympus Mons Aureole: PSP_003806_1975 ESP_012627_1975 (Interval in Earth days: 687) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.32 | 217. | 2.81 | 19.24 | 61.8 | 61.8 |
| Mangala Valles Cataract: PSP_003991_1645 PSP_004347_1645 (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 | -15.3 | 210. | 0 | 10.73 | 46.2 | 41.2 |
| Exposure of South Polar Layered Deposits: PSP_004996_1065 PSP_005339_1065 (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 | -73.0 | 145. | 2.20 | -14.7 | 56.6 | 61.3 |
| Gullies: PSP_003954_1445 PSP_004231_1445 (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 | -34.9 | 144. | -5.8 | -28.8 | 45.1 | 43.4 |
| Unnamed Well-Preserved Crater within the Isidis Basin: PSP_003560_1900 PSP_005828_1900 (Interval in Earth days: 177) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 10.16 | 94.5 | 0.61 | 10.89 | 58.6 | 37.6 |
| Layered Deposit in Crommlin Crater: PSP_003432_1850 PSP_005766_1850 (Interval in Earth days: 182) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.980 | 350. | -7.0 | -19.9 | 57.3 | 38.0 |
| Streamlined Form in Kasei Valles: PSP_003408_1990 PSP_003698_1990 (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 | 18.90 | 283. | -4.4 | 23.25 | 62.9 | 61.3 |
| Light-Toned Outcrops in the Plains Between Melas and Candor Chasma: PSP_004318_1730 PSP_004740_1730 (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 | -6.84 | 282. | -3.1 | -15.3 | 45.8 | 41.7 |
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