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Jupiter Image 2022/10/11(UT)
鈴木邦彦,佐藤康明,高松 泉,堀川邦昭,阿久津富夫
Eric Sussenbach,Gary Walker,Christopher Go,Yaroslav Naryzhniy,Niall MacNeill,Vincenzo della Vecchia,Randy Tatum,Michel Jacques Jacquesson,Jean-Paul OGER,Jean-Luc Dauvergne,Cristina Cellini,Rudolf A.Hillebrecht,Paulo Casquinha,Efrain Morales Rivera
K.Suzuki,Y.Sato,E.Sussenbach,G.Walker,Christopher Go,I.Takamatsu,Y.Naryzhniy,K.Horikawa,N.MacNeill,T.Akutsu,V.della Vecchia,R.Tatum,Michel.J,Jean-Paul.O,JL Dauvergne,C.Cellini,R.A.Hillebrecht,P.Casquinha,E.Morales
ひまわり画像的には無理かと思っていましたが、
雲間から大赤斑を撮像できました。
2枚目あたりは気流も悪くなかったです
[Kunihiko Suzuki : Yokohama-city Kanagawa-Prefecture Japan]
≪神奈川県 横浜市 鈴木邦彦≫
薄雲の通過があり光度が安定しませんでした
-----------------------------------------------------
[Sagamihara-shi Kanagawa-prefecture Japan]
≪神奈川県相模原市 佐藤康明≫
[Eric Sussenbach : [ Willemstad,Curacao (Dutch Caribbean)]
The seeing was poor.
[Gary Walker:Georgia:USA]
We had a powerful thunderstorm early this evening. Surprisingly the sky cleared up at around 8pm.
However seeing and transparency wasn't very good.
The GRS is well resolved. The wake of the GRS is very complex and seem to be spilling into the STrZ!
This is a bit weird. This may be due to an outbreak very close to the halo of the GRS.
The chimney above the GRS seem to be closing.
Note the very bright white cyclonic oval on the STB close to the CM.
Note the outbreaks of the NEBs.
It seems it is these small and short term outbreaks that is slowly reviving the NEB.
At the NPR,2 white ovals can be seen. These are the polar ovals that Juno images during Perijove.
[Christopher Go : Cebu Philippines]
≪高松 泉 : ≫[Izumi Takamatsu: Arakawa,Tokyo,Japan]
Seeing 6/10 Trans 7/10
IR 19:37 UTC
[Yaroslav Naryzhniy : Ukraine,Kiev region]
STrBの先端はII=116°まで進み、出発点である大赤斑後部のフックが見えるところまで来ました。
先端は少し拡散して、CMTが取りにくくなっています。
SEB南縁は暗斑だらけで活動的ですが、post-GRS dist.は短くなって、少し静かになってきたようです。
≪神奈川県横浜市泉区 堀川邦昭≫[Kuniaki Horikawa:Kanagawa Japan]
I made RGB and IR 642nm BP runs on Jupiter with the GRS in transit on 11th October 2022.
The seeing looked quite good,with few visible large perturbations on the planet's disk on the video feed.
However,there was a shimmer which I believe was due to short wavelength,higher frequency turbulence.
In the final processing this pretty much wiped out the very fine detail.
The seeing improved by the time I then moved over to Methane band and was better again for the 2nd RGB
and IR 642nm BP runs,with the GRS closer to the Central Meridian.
However,again the resolution of very fine detail was impacted.
[Niall MacNeill : Wattle Flat,NSW,Australia]
セブ島からのルーチン画像です。
≪茨城県 : 阿久津富夫≫
[Vincenzo della Vecchia : [Aversa,Italy]
[ Randy Tatum,Richmond,VA U.S.A]
[Michel Jacquesson : Sevigny-Waleppe (Ardennes) France]
[Jean-Paul OGER : France]
[Jean-Luc Dauvergne:Paris France]
[Cristina Cellini : San Romualdo - Ravenna,Italy]
Jupiter with Io in transit and its shadow under fair to good seeing with my refractor.
[Rudolf A.Hillebrecht: Bad Gandersheim,Germany ]
(site: 38.567 N /8.933 W Alt 124 m)
[Paulo Casquinha Palmela,Portugal]
[Efrain Morales Rivera Aguadilla:Puerto Rico]
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