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Saturn Image 2020/07/21(UT)
Vincenzo della Vecchia,Christofer Mauricio Baez Jim,Peter Edwards,Trevor Barry,Constantin Sprianu,Michael Wong,Vlamir da Silva Junior
V.della Vecchia,C.Baez,P.Edwards,T.Barry,C.Sprianu,M.Wong,V.da Silva Jr.
This image comes from 5 IR's stack.
[Vincenzo della Vecchia : [Aversa,Italy]
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Christofer Mauricio Baez Jimenez |
19 images derotated using WinJUPOS.
[Christofer Mauricio Baez Jimenez :Santo Domingo,Dominican Republic.]
[Peter Edwars: West Sussex United Kingdom]
All data was captured through a thin veil of cloud which dropped the histogram for each channel about 20 to 30% but the live feed was stable with crisp detail. Quite surprising detail is resolved in all data,the 685nm IR well resolves the North polar vortex and vertices of the hexagon. The thin concentric banding structure within the North polar collar is well resolved in IR and R channel data. A compact dark spot is resolved in IR and R data at approx Lat+59.9 L3 172.7 and a large diffuse spot is resolved within the polar collar in the RGB data at approx Lat+62 L3 160.9
[Trevor Barry:Broken Hill:Australia]
in very bad conditions
[Constantin Sprianu,Otopeni,Romania]
[Michael Wong,Hong Kong,China]
some hours after the opposition which happened on July 20th. The rings are very bright compared to the disc, the Seeliger Effect.
[Vlamir da Silva Junior : Sao Paulo,Brazil]
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