–د ALPO-Japan Latest
Jupiter Image 2021/05/04(UT)
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Clyde Foster,Jose Luis Pereira,Vinicius Mansano Martins,Lucca Schwingel Viola,Vlamir da Silva Junior
C.Foster,J.Luis,K.Suzuki,V.Martins,S.Viola,T.Akutsu,K.Horikawa,V.da Silva Jr.
GRS was transiting,but conditions were unfortunately rather poor.
It appears that the dark circulating loop may have been disturbed (possibly by the SEBs ring?).
There may be a slight "bump" on the sf edge of the GRS and if there is going to be a secondary flake appearing on the sp edge,
I would expect it quite soon (no guarantees,but it wouldnft surprise mec.
[Clyde Foster:Centurion,South Africa]
[Jose Luis Pereira :Sao Caetano do Sul/Sao Paulo/Brasil]
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[Kunihiko Suzuki : Yokohama-city Kanagawa-Prefecture Japan]
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2021-05-04 (yyyy-mm-dd),08:13.6 UT CM I 306,2‹ CM II 215,6‹ CM III 10,4‹
Seeing 3/10 Trans 8/10
[Vinicius Mansano Martins : Ribeirao Preto - SP,Brazil]
2021-05-04 (yyyy-mm-dd),07:26.6 UT CM I 277,5‹ CM II 187,2‹ CM III 342,0‹
Seeing 7/10 Trans 10/10
[Lucca Schwingel Viola : Matupa Brazil]
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á_“Þ쌧‰¡•lŽsò‹æ –xì–Mºâ[Kuniaki Horikawa:Kanagawa Japan]
Transit of Oval BA. In one of the images it's close to the CM. We can see the center of it as a pinpoint difference in color.
It's possible to observe the cyclonic area to the right of Oval BA. A1, A2, A3, A4 and A5,
are all these white ovals visible at least in one of the images on SSTeB.
SEB is divided in two. NEB is pale mainly in most of its northern area.
A prominent white oval is well visible on NEBn 'following side' together with a barge.
A barge is also visible on the 'preceding side' of this belt. NTB is also well visible and divided in two.
[Vlamir da Silva Junior : Sao Paulo,Brazil]