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: PSP_006821_1270 ESP_024121_1270 (Interval in Earth days: 1349) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -52.6 | 351. | -0.1 | -25.5 | 68.9 | 63.9 |
| Exposure of Polar Layered Deposits within Southern Residual Cap: PSP_005029_0930 PSP_005239_0930 (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 | -86.8 | 11.6 | 0.89 | 15.20 | 68.5 | 69.6 |
| 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 |
| Large Fresh Crater Near Marte Vallis: PSP_006985_2020 PSP_009912_2020 (Interval in Earth days: 228) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.51 | 184. | -2.8 | -22.3 | 39.3 | 50.3 |
| Cone in Chasma Boreale: PSP_006901_2610 PSP_006980_2610 (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 | 80.99 | 300. | -5.0 | 0 | 74.2 | 72.8 |
| Surface Morphology: PSP_005935_2275 ESP_011855_2275 (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 | 46.90 | 49.0 | 0.36 | 19.26 | 61.4 | 73.1 |
| Layered Deposits in Impact Crater in Utopia Planitia: PSP_006606_2240 PSP_007041_2240 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 43.81 | 89.5 | -5.9 | 16.71 | 51.1 | 45.7 |
| Ithaca Region Defrosted: PSP_004666_0945 PSP_004891_0945 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -85.2 | 181. | -0.9 | -18.0 | 64.2 | 67.5 |
| Seasonal Monitoring: PSP_005708_0940 ESP_047191_0940 (Interval in Earth days: 3232) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -85.9 | 178. | 1.06 | 22.84 | 76.8 | 76.8 |
| Tomini Crater Western Ejecta: PSP_005695_1965 PSP_005985_1965 (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 | 16.25 | 125. | -1.0 | 26.25 | 42.8 | 38.2 |
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