木星 ALPO-Japan Latest

Jupiter Image 2018/06/26(UT)
鈴木邦彦,堀川邦昭
Christopher Go,Avani Soares,Gregory H. Revera,Jean-Luc Dauvergne,Pericles Enache,George Lamy,Frank J Melillo,Christophe Pellier,Marc Delcroix
K.Suzuki,Christopher Go,A.Soares,G.Revera,K.Horikawa,JL Dauvergne,P.Enache,G.Lamy,Frank,Christophe.P,M.Delcroix

Kunihiko Suzuki
強風と雲と劣悪なシーイングでした。
それでも大赤斑はやはりいいものです。

[Kunihiko Suzuki : Yokohama-city Kanagawa-Prefecture Japan]
≪神奈川県  横浜市  鈴木邦彦≫

Christopher Go
I had a late imaging run for Jupiter today.   Seeing was variable.
Oval BA is on the left while the STB shows the wake and the remnant of the STB Ghost.  
Note the very large white oval on the NW of Oval BA. This feature is getting close to Oval BA!
In the south pole,there is a bright streak which is very obvious in the IR pass image. The EZ has a strong ochre color. The NEB and SEB are quiet in this region. [Christopher Go : Cebu Philippines]

Avani Soares
Keeping the insistence even with medium seeing,it was only 5 movies and the clouds closed everything,only that was saved. 
It had been a long time since I had captured Oval BA clearly. [ Observatory Parsec,City Canoas,Brazil]

Gregory H. Revera
2018 June 26
02:07:54UT
I:   22.9°
II:  332.3°
III: 209.6°

[Gregory H. Revera : Madison,Alabama,USA]

Kuniaki Horikawa
風が強く、シーイングも真冬のようで悪くなる一方でした。

≪神奈川県横浜市泉区  堀川邦昭≫[Kuniaki Horikawa:Kanagawa Japan]

Jean-Luc Dauvergne



[Jean-Luc Dauvergne:Paris France]

Pericles Enache
Seeing and transparency were very good but,occasionally,a jet stream
affected the atmosphere with some turbulance,which was not bad
enough.

I produced 3 observations in visible light and another one in CH4 20
nm band. It was my first attempt using this filter but I think the
result is reasonable taking in consideration the modest apperture of C8.




[Pericles Enache,Sao Paulo,Brazil]

George Lamy

[George Lamy,springfield,louisiana,USA]

Frank J Melillo

[Frank J Melillo  Holtsville NY U.S.A]

Christophe Pellier
Some Images of the GRS on June 26th mainly. Many of us are wondering if the pinching of the STrZ at p.part is the reborned STrD,these images still don't bring an answer,although the UV image unexpectedly reveals a dark bridge
Of note again in UV is the very strong contrast of the Equatorial "band",now equal to that of the NEB!





[Christophe Pellier  Bruz City,France]

Marc Delcroix




[Marc Delcroix  Tournefeuille,France]

ALPO-Japan Latest Jupiter Section
2018/06/27
2018/06/25