木星 ALPO-Japan Latest
Jupiter Image 2018/08/14(UT)
江口利哉,鈴木邦彦,井上 修,皆川伸也,村田孝昭,永長英夫
Trevor Barry,Clyde Foster,Joaquin Camarena,Pericles Enache,Michel Jacquesson,Manos Kardasis
T.Eguchi,K.Suzuki,O.Inoue,N.Minagawa,T.Murata,H.Einaga,T.Barry,C.Foster,J.Camarena,P.Enache,Michel.J,Kardasis
≪東京都杉並区 江口利哉≫[T.Eguchi : Suginami Tokyo Japan]
貴重な晴れ間なので、シーイング悪化は承知の上で3枚撮影しました。
さすがに3枚目はぶよぶよでした。
[Kunihiko Suzuki : Yokohama-city Kanagawa-Prefecture Japan]
≪神奈川県 横浜市 鈴木邦彦≫
≪大阪府 枚方市 井上 修≫[Osamu Inoue. Hirakata-shi,Osaka,Japan]
シーイング、透明度ともにまずまずでした。LRGB3セットをDe-Rotationしました。
≪東京都 立川市 皆川伸也≫[Nobuya Minagawa:Tokyo Japan]
≪東京都 国立市 村田孝昭≫[Takaaki Murata: Tokyo Japan]
[Hideo Einaga Kasai-City Hyogo-Prefecture Japan]
≪兵庫県 加西 永長英夫≫
Imaged Jupiter Aug 14th,had good transparency but the jet prediction was very crook and that is how it panned out.
Only have a very early 685nm IR.
Rather surprisingly the level of detail seems quite fair especially so in the region of oval BA,
only stacked 50% of the available data.
[Trevor Barry:Broken Hill:Australia]
RGB and IR image set from yesterday evening with the GRS central. As per Christophe Pellier’s recent comment to me,it does appear that the turbulence following the GRS may be reduced/reducing. I also note the triplet of reddish spots in the SPR.
[Clyde Foster:Centurion,South Africa]
[Joaquin Camarena:Spain]
Conditions were not so great with lower haze and turbulence in high
atmosphere. I could get 6 RGBs sequences in a row,out of 20,that
were reasonable to process and de-rotate in 9 minutes. From these 6
RGB sequences,the best RGB sequence was recorded at 22:48 UT,showing
Ganymede close to Jupiter,attached at this report,as well.
[Pericles Enache,Sao Paulo,Brazil]
[Michel Jacquesson : Sevigny-Waleppe (Ardennes) France]
[Manos Kardasis,Glyfada-Athens;Greece]
《カーダシス マノス:ギリシャ アテネ》