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.
| Landslide Scarp: PSP_007785_1645 PSP_008141_1645 (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 | -15.1 | 303. | 7.47 | -3.79 | 56.0 | 60.0 |
| Fault Relays in the Cerberus Fossae: PSP_007645_1885 PSP_007856_1885 (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 | 8.465 | 164. | -5.5 | -23.3 | 43.9 | 46.8 |
| Floor and Central Uplift of Mazamba Crater in Thaumasia Planum: PSP_007100_1520 ESP_033248_1520 (Interval in Earth days: 2038) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.5 | 290. | -1.6 | -23.6 | 55.6 | 51.8 |
| Middle Section of Northern Olympus Mons Basal Scarp: PSP_007089_2035 PSP_007946_2035 (Interval in Earth days: 67) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.25 | 223. | 7.43 | -6.64 | 38.8 | 42.1 |
| Region Showing Differentially-Eroded Distal Fan Deposits: PSP_007688_1575 PSP_008545_1575 (Interval in Earth days: 67) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -22.0 | 72.9 | 6.99 | -15.6 | 59.4 | 68.1 |
| Light-Toned Layered Deposits Along Plains South of Ius Chasma: PSP_007786_1710 PSP_009935_1710 (Interval in Earth days: 167) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.74 | 276. | -4.8 | 20.55 | 52.9 | 58.8 |
| Thinly-Banded Light-Toned Rock in Unnamed North Sinus Meridiani Crater: PSP_007084_1845 PSP_007440_1845 (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 | 4.433 | 2.80 | 3.48 | -6.89 | 39.8 | 43.7 |
| Fan in Aeolis Region: PSP_007975_1755 PSP_009623_1755 (Interval in Earth days: 129) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.65 | 154. | -4.9 | 5.617 | 52.4 | 57.8 |
| Area Near Summit of Gale Crater Mound: PSP_008002_1750 PSP_009927_1750 (Interval in Earth days: 151) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.85 | 137. | -5.8 | -22.8 | 52.8 | 59.9 |
| Lineated Valley Fill in Deuteronilus Mensae: PSP_007795_2175 PSP_009588_2175 (Interval in Earth days: 140) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 37.35 | 24.6 | -4.2 | 7.505 | 42.0 | 44.3 |
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