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Saturn Image 2007/04/10(UT)
米山誠一,瀧本郁夫
Ralf Vandebergh
S.Yoneyama,R.Vandebergh,I.Takimoto
|
Seiichi Yoneyama(200mm Newton) |
≪神奈川県横浜市 米山誠一≫
|
Ralf Vandebergh(250mm Newton) |
One of my most detailed observations of the Saturn atmosphere.
The animation shows immediately a very turbulent EB,which seems
to have a wavy appearance.Also a wealth of other smaller structure
can be seen moving with the rotation.
The air was very steady,thanks to the nearby high pressure region
in the neighbourhood of the UK.(observing location: south of the
Netherlands).
10in Newton/ATK-1HS)
L3=97--105 red light 610nm)
One of my most detailed observations of the Saturn atmosphere.
The animation shows immediately a very turbulent EB,which seems
to have a wavy appearance.Also a wealth of other smaller structure
can be seen moving with the rotation.
The air was very steady,thanks to the nearby high pressure region
in the neighbourhood of the UK.(observing location: south of the
Netherlands).
10in Newton/ATK-1HS)
The turublent shape of the EB as reported earlier seems to
be connected with clear cloud-structure within the EZ-s,
as seen in these animations.
Additional: a color result from the same day(RT-RGB)
Note the fine appearance of the STrZ.
[バンディバ:オランダ]
[Ralf Vandebergh:Neighbourhood of Maastricht Netherlands]
|
Ikuo Takimoto (310mm Newtonian) |
コメント：昨日よりもシーイングが改善した。異変は無いようだ。
[Ayauta-gun Kagawa-Prefecture Japan]
≪香川県 綾歌郡 瀧本郁夫≫
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