木星 ALPO-Japan Latest
Jupiter Image 2020/03/16(UT)
鈴木邦彦,荒川 毅,堀川邦昭,井上 修
Clyde Foster,Vincenzo della Vecchia,Trevor Barry,Christopher Go,Vlamir da Silva Junior
C.Foster,V.della Vecchia,K.Suzuki,T.Arakawa,K.Horikawa,O.Inoue,T.Barry,Christopher Go,V.da Silva Jr.
I just managed a single RGB this morning,which didn't come out too badly.
[Clyde Foster:Centurion,South Africa]
Another attempt at Jupiter this morning,unfortunately in quite bad seeing conditions.
[Vincenzo della Vecchia : [Aversa,Italy]
[Kunihiko Suzuki : Yokohama-city Kanagawa-Prefecture Japan]
≪神奈川県 横浜市 鈴木邦彦≫
≪奈良県奈良市 荒川 毅≫[Tsuyoshi Arakawa:Nara Japan]
≪神奈川県横浜市泉区 堀川邦昭≫[Kuniaki Horikawa:Kanagawa Japan]
≪大阪府 枚方市 井上 修≫[Osamu Inoue. Hirakata-shi,Osaka,Japan]
Imaged Jupiter March 16th in quite nice seeing for the altitude.
All data was captured with Jupiter below 40 degrees.
I note the quite extravagant festoon in the EZ,the chimney above the GRS is most definitely open. Of great interest is the morphology of the SEB either side of the GRS.
To the P side of the GRS the SEB is quite smooth but to the F side is chaotic and seems 3 dimensional.
Within this structure there appear to be high altitude plumes,these are well seen in the Ch4 data.
The Sun is shining on the surface from the F side and the these plumes seem to have shadow thrown to the P side indicating the height of these structures.
When comparing these data with my data from March 11th the structure to the F side of the GRS has evolved significantly.
[Trevor Barry:Broken Hill:Australia]
Seeing was good when I started imaging.
I started taking IR and CH4 images thinking that seeing would even be better when Jupiter gets higher.
Unfortunately,seeing deteriorated as the sun was about to rise.
Oval BA can be seen in these images. It is still white.
The SEBn is very active while the rest of the SEB looks pale.
The mid=EZ is very bright in methane band this year.
The NEB is dark and narrow.
[Christopher Go : Cebu Philippines]
[Vlamir da Silva Junior : Sao Paulo,Brazil]