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.
| Scallops and Polygons: PSP_001582_2245 PSP_002848_2245 (Interval in Earth days: 99) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 44.35 | 86.4 | 1.92 | 11.02 | 51.4 | 68.6 |
| Delta in Crater South of Parana Basin: PSP_001388_1565 PSP_001586_1565 (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 | -23.5 | 347. | -2.1 | -16.1 | 67.0 | 66.9 |
| Field of Morphologically-Diverse Ring/Cone Structures in Athabasca Valles: PSP_001606_1900 PSP_002226_1900 (Interval in Earth days: 48) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.645 | 156. | 4.90 | -25.6 | 51.3 | 56.5 |
| Multiple Episodes of Gully Formation, As Seen in MOC Image R16-02071: PSP_002002_1390 PSP_002846_1390 (Interval in Earth days: 66) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -40.7 | 155. | 8.34 | -14.7 | 71.6 | 62.7 |
| Possible Location of Viking Lander 2: PSP_001976_2280 PSP_002055_2280 (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 | 47.65 | 134. | -1.1 | 21.16 | 57.9 | 57.2 |
| Crater with Gullies, Debris Mantle, Layers Exposed in Eastern Wall: PSP_001948_2140 PSP_002238_2140 (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 | 33.85 | 181. | -3.1 | 20.48 | 54.0 | 55.5 |
| Pristine-Looking Gully : PSP_002692_2295 PSP_002824_2295 (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 | 49.13 | 25.2 | 5.98 | -20.2 | 69.0 | 73.1 |
| Lobate Debris Apron: PSP_001570_2215 PSP_001834_2215 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.99 | 54.6 | -0.1 | -21.0 | 50.7 | 55.7 |
| East Mareotis Tholus: PSP_001364_2160 PSP_001760_2160 (Interval in Earth days: 31) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.89 | 274. | 1.07 | -21.4 | 48.0 | 53.8 |
| Landslides on Flat Topography in Elysium Planitia: PSP_001593_1875 PSP_002437_1875 (Interval in Earth days: 66) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.187 | 151. | -1.9 | 22.92 | 52.5 | 53.2 |
Page 875 of 891 (8,901 images) | |||||