木星 ALPO-Japan Latest
Jupiter Image 2020/07/08(UT)
Guilherme Grassmann,Javier Beltran Jovani,Michel Jacquesson,Randy Tatum,Clyde Foster,Michael Wong,Ecleido Sousa Azevedo,Jean-Luc Dauvergne,Vlamir da Silva Junior,Trevor Barry,Niall MacNeill
G.Grassmann,Javier,Michel.J,R.Tatum,K.Sasaki,C.Foster,M.Wong,E.S.Azevedo,JL Dauvergne,V.da Silva Jr.,T.Barry,N.MacNeill
[Guilherme Grassmann,Americana-San Paulo,Brasil]
[Javier Beltran Jovani:Castellon-Spain]
[Michel Jacquesson : Sevigny-Waleppe (Ardennes) France]
Under a mostly cloudy sky,Jupiter was in a clear patch. Low altitude and local heating affected seeing.
[ Randy Tatum,Richmond,VA U.S.A]
[K.Sasaki:Ohsaki-City Miyagi-Prefecture Japan]
Poor seeing conditions as we have a large cold front system approaching.
Still hoping for some better opportunities over opposition.
[Clyde Foster:Centurion,South Africa]
[Michael Wong,Hong Kong,China]
[Ecleido Sousa Azevedo : Areado/MG,Brasil]
[Jean-Luc Dauvergne:Paris France]
Clyde's spot has risen in these images. GRS and A8 is rising. Near the CM we can see A7 (SSTB).
Note also,almost invisible S3-AWO-2. The seeing allowed a good registration of LRS-1 on NNTB/Z area,
on the following side,and also another spot to the right and north of it,near the CM.
We can see the f. end of NTB(N). NEB much darker than SEB here in general.
Some spots on SEBs,the same latitude of the GRS,a notable one setting.
[Vlamir da Silva Junior : Sao Paulo,Brazil]
Imaged Jupiter July 8th targeting the region between Oval BA and the GRS.
Seeing was good initially for the IR data until the cloud rolled in.
Most of the R,G & B data was effected to some extent by cloud. A nice depth of fine detail is resolved in the NPR.
I note an interesting very faint medium size oval in the NNTZ just below the NTB near the CM at the beginning of the session,resolved in IR,R & RGB but best seen in Ch4.
The structure in the NEB is quite intricate with two prominent dark features extending down into the EZ.
The GRS chimney is open and the structure trailing it in the SEB is well resolved.
The dark formation following Oval BA is well resolved as are the compact dark spots above and below.
There is a small spot in the SSTB below the GRS and small red oval very far South on the edge of the SPR which is quite bright in Ch4.
[Trevor Barry:Broken Hill:Australia]
[Niall MacNeill : Wattle Flat,NSW,Australia]