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 in Southern Latitude Crater: PSP_005701_1445 PSP_005991_1445 (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 | -35.2 | 328. | 0.44 | 26.02 | 39.3 | 41.2 |
| Ringed Pit in Tractus Fossae: PSP_005677_2055 ESP_011597_2055 (Interval in Earth days: 462) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.97 | 256. | -3.0 | 22.36 | 49.0 | 60.5 |
| Light-Toned Outcrops in Noctis Labyrinthus: PSP_006692_1740 ESP_024427_1740 (Interval in Earth days: 1382) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.99 | 267. | 1.10 | 14.97 | 39.0 | 37.4 |
| Graben in Eastern Olympus Mons: PSP_005678_1995 PSP_005744_1995 (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 | 19.44 | 230. | -7.4 | -26.8 | 45.5 | 46.1 |
| Small Fresh Crater: PSP_005567_1690 ESP_023948_1690 (Interval in Earth days: 1432) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -10.6 | 24.5 | -11. | 8.2 | 33.9 | 34.3 |
| Diverse Stratigraphic Layers Exposed in Depression: PSP_006290_1590 PSP_010575_1590 (Interval in Earth days: 334) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -20.8 | 85.3 | 0 | 16.21 | 39.8 | 63.6 |
| Central Uplift in Runanga Crater: PSP_006620_1530 PSP_010549_1530 (Interval in Earth days: 306) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -26.6 | 75.8 | 0.19 | 16.27 | 47.6 | 66.7 |
| Large Unnamed Fresh Crater West of Tomini Crater: PSP_005748_1980 PSP_006671_1980 (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 | 18.00 | 118. | 4.14 | -5.01 | 43.2 | 38.6 |
| Basal Exposure of South Polar Layered Deposits: PSP_005049_1075 PSP_005247_1075 (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 | -72.1 | 138. | 1.11 | -21.4 | 56.5 | 60.0 |
| 36 Gullies Previously Identified and Fully Described in MOC Image M03-03547: PSP_005646_1360 ESP_022682_1360 (Interval in Earth days: 1327) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -43.7 | 34.1 | -24. | -7.08 | 45.2 | 38.1 |
Page 855 of 913 (9,124 images) | |||||