木星 月惑星研究会 関西支部

Jupiter Image 2004/11/24(UT)
瀧本郁夫,
Ralf Vandebergh,Paulo Casquinha
I.Takimoto,R.Vandebergh,P.Casquinha

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2004/11/24 20:21:23(UT)
I=212.2 II=215.9 III=214.7
De= -2.6 E.Dia=32.69"
15fps AVI 90sec 1043/1349frams Stacked
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2004/11/24 20:32:45(UT)
I=219.1 II=222.8 III=221.6
De= -2.6 E.Dia=32.69"
15fps AVI 90sec 949/1349frams Stacked
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2004/11/24 20:43:37(UT)
I=225.7 II=229.4 III=228.1
De= -2.6 E.Dia=32.69"
15fps AVI 90sec 960/1349frams Stacked
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2004/11/24 20:53:48(UT)
I=232.0 II=235.5 III=234.3
De= -2.6 E.Dia=32.69"
15fps AVI 90sec 1069/1350frams STacked
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2004/11/24 21:11:13(UT)
I=242.6 II=246.0 III=244.8
De= -2.6 E.Dia=32.69"
15fps AVI 90sec 714/1349frams Stacked
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コメント：気流が悪い、詳細不明。
[Ayauta-gun Kagawa-Prefecture Japan]
≪香川県  綾歌郡  瀧本郁夫≫

Thanks moderate seeing with no wind I could take this image,my first Jupiter image of the apparition.
The area of the GRS is visible well,also some nice structures with festoons within the NEB.
Taken with the ToUcam at 0.25´´ per pixel.Seeing ca 7/10.Jupiter still rising.


Here is another image of Jupiter taken on nov 24 in a moment of better air,and in almost daylight brightness.
There are already a few white ovals visible within the STeB,also within the SSTeB which is clearly
divided by the STeZ.(pretty distorted of shape)Also the SSTeZ and the SPB are seperated visible.


Hi all,

I have one image from november 24 showing the white oval BA,now 4/5 months after the encounter with the GRS.
I thought it would be interesting how the appearance of the BA looks.The distance to the GRS is already passable
large.The seeing during this image was poor,due to Jupiter's low position in the sky.


[バンディバ:オランダ]
[Ralf Vandebergh:neighbourhood of Maastricht Netherlands]

ALPO-Japan Latest Jupiter Section