Mars Image 2022/03/27(UT)
Clyde Foster,Carsten Bauer
C.Foster,C.Bauer
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| Clyde Foster |
I had variable seeing this morning with some cloud interference. The RGB is produced from the single best channel images. Unfortunately the longer wavelength channels are severely affected by edge artefact, which is likely exacerbated by the eastern boundary of Elysium (Phlegra, Trivium Charontis and Cerberus) being very close to the limb. Olympus Mons is at lower left, with some nice late afternoon equatorial cloud over the Tharsis Montes region[Clyde Foster:Centurion,South Africa]
| Carsten Bauer | |
The morning air was a bit clearer than the days before, but unfortunately still as turbulent. So again no chance for a useful B image. But this time the SPC/SPH can be identified in G. Also interesting are the small bright patches near the evening terminator in the R image (top right). This should be the region of Olympus Mons and Tharsis. While both are certainly not distinguishable directly in this low resolution, with low sunlight incidence and long shadows there probably might be situations in which their presence in the Martian landscape becomes noticable at a greater scale ?[Carsten Bauer : Frankfurt,Germany]
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