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.
| 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 |
| Potentially Very Recent Impact Markings: PSP_005693_1650 ESP_011468_1650 (Interval in Earth days: 450) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.6 | 184. | 1.26 | 15.00 | 32.9 | 57.3 |
| Mcmurdo Crater on the South Polar Layered Deposits: PSP_004646_0955 PSP_004884_0955 (Interval in Earth days: 18) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -84.4 | 1.54 | 0 | -18.3 | 63.4 | 66.4 |
| Dry Cataract in Lethe Vallis: PSP_006762_1840 PSP_010335_1840 (Interval in Earth days: 278) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.744 | 155. | -7.4 | 7.064 | 38.2 | 54.1 |
| Fresh High-Latitude Crater: PSP_006924_2335 PSP_009864_2335 (Interval in Earth days: 230) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 53.11 | 44.5 | -0.5 | 18.47 | 53.5 | 47.5 |
| 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 |
| Large Shallow Crater on Edge of South Polar Layered Deposits: PSP_005390_0935 PSP_005666_0935 (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 | -86.5 | 232. | -1.3 | 14.58 | 72.8 | 75.6 |
| Arandas Crater in Northern Plains: PSP_006267_2230 ESP_019545_2230 (Interval in Earth days: 1035) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 42.40 | 345. | 0 | 10.33 | 53.7 | 54.1 |
| 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 |
| 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 |
Page 852 of 900 (8,995 images) | |||||