木星 ALPO-Japan Latest

Jupiter Image 2020/05/13(UT)
鈴木邦彦,荒川 毅,井上 修,熊森照明,堀井恵策
Clyde Foster,Christopher Go,Anthony Wesley,Trevor Barry,Cory Schmitz,Efrain Morales Rivera,George Lamy,Andy Casely,Niall MacNeill,Vlamir da Silva Junior
C.Foster,K.Suzuki,T.Arakawa,Christopher Go,Anthony.W,T.Barry,O.Inoue,C.Schmitz,T.Kumamori,E.Morales,K.Horii,G.Lamy,A.Casely,N.MacNeill,V.da Silva Jr.

Clyde Foster
A short,frustrating session with plenty of cloud interference and poor seeing,allowing just enough data capture for this RGB. No IR or CH4

[Clyde Foster:Centurion,South Africa]

Kunihiko Suzuki
雲が多く、シーイングも劣悪でした。結局日の出前に1枚のみ記録です

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

Tsuyoshi Arakawa

≪奈良県奈良市  荒川 毅≫[Tsuyoshi Arakawa:Nara Japan]

Christopher Go
The outer bands of Typhoon Vongfong (Ambo) has reached us.
I was fortunate to get a short clearing before the sky was overcast.
Transparency was very poor due to thin clouds.  Seeing was fair.

Oval BA is still pale and a hint of the inner dark ring can be seen.
The SEB has lost its color and is no pale red.  The NEB is very chaotic.
I have never seen it like this before.  Is the NEB fading?  Is it undergoing an upheaval?

Note:CM3 of IR image  × 222 --> 〇 122

[Christopher Go : Cebu Philippines]

Anthony Wesley
Hi all,here are three images of Jupiter from this morning in overall
poor seeing. Once again the IR750 image holds up the best but the RGB is
low resolution thanks to the strong jetstream that's presently over my
location.

The GRS can be seen setting at lower right,with Oval BA rising at lower
left. The red spot in the STZ can be seen close to centre to bottom. The
North Equatorial Belt is very active,a lot of storm activity is visible
near the centre of the image at top,and it takes on the odd bubble-like
appearance off to the left that it's been showing recently.

The methane absorption image (CH4) shows the area around the GRS to be
relatively unchanged,and there are a number of isolated high altitude
spots visible as well as the normal polar hazes. There is a marked
difference in appearance between the North and South Equatorial Belts,
the SEB appears almost uniformly dark in CH4 whereas the NEB shows many
brighter regions indicating a lot of high altitude clouds.






[Anthony Wesley,Murrumbateman Australia]
≪アンソニ  オーストラリア≫

Trevor Barry





[Trevor Barry:Broken Hill:Australia]

Osamu Inoue

≪大阪府  枚方市  井上  修≫[Osamu Inoue. Hirakata-shi,Osaka,Japan]

Cory Schmitz
Conditions were quite bad at this time,as thin clouds were moving through the field of view.
Illumination kept changing as a result. Conditions in general were quite poor.

[Cory Schmitz : Johannesburg,South Africa]

Teruaki Kumamori
黄砂もいなくなり、透明度良くまずまずのシーイングとなりました



≪大阪府堺市 熊森照明≫[Teruaki Kumamori:Ohsaka Japan]

Efrain Morales Rivera




[Efrain Morales Rivera  Aguadilla:Puerto Rico]

Keisaku Horii

≪兵庫県姫路市  堀井恵策≫[Keisaku Horii : Himeji Hyougo Japan]

George Lamy

[George Lamy,springfield,louisiana,USA]

Andy Casely



[Andy Casely,Sydney,Australiaa]

Niall MacNeill

[Niall MacNeill : Wattle Flat,NSW,Australia]

Vlamir da Silva Junior

[Vlamir da Silva Junior : Sao Paulo,Brazil]

ALPO-Japan Latest Jupiter Section
2020/05/14
2020/05/12