土星撮像後更に雲が厚くなる。
疲れで暫く仮眠後、望遠鏡を片付けにかかる。更に雲が厚くなり月には暈すらかかっている。
木星以外には星は見えないが、試しに更に拡大率を低くして撮像してみた。
このような状況での撮像は初めてであった。
透明度が極めて悪いながらも、この位迄拡大率をおとせば撮像出来ることがわかっただけでも収穫。
[Kenkichi Yunoki  (Sakai City  Japan)]
≪大阪府  堺市  柚木健吉≫

1200frames composite
Seeing:7/10,Trans1/5

This picture was taken through thin clouds.
In the pictures of this term, it is the one where resolution is higher.

≪埼玉県上尾市  仁科淳良≫

撮影し始めた頃はうす曇であったが、次第に雲が厚くなり中断。
最終撮影時は合成F値を少し下げて光量を稼ぎました。
シーイングは良好だったのに残念な一夜でした。

2004/03/08 11:24:12(UT) 〜13:31:39(UT)
I=109.7 II=307.6 III=235.7 〜I=187.4 II= 24.7 III=312.8
[Yukio Oshihoi  (Hirakata-City Oosaka-Prefecture  Japan)]
≪大阪府 枚方市　忍穂井幸夫≫

≪群馬県佐波郡  冨田安明≫

I attache Jupiter images on 08 March  2004
NEBs Festoon is very active. Two dark area of SEBs(about II=0-10) are very prominent by IR image

Image data        08 March 2004

ToUcam         600 frames    exposure　1/33seconds
UV               　9-18frames   exposure  5-7seconds   2x2bining 　　                          　
IR(800nm)       14-38frames　exposure　0.5-1seconds     2x2bining                        　                              　
METHANE      13-20frames    exposure   10-15seconds     2x2bining

S=5-6/10    T=4-5/5

≪栃木県  阿久津富夫≫

・SEBn、NEBとも活発な活動を呈しています。
HIDEO EINAGA ≪兵庫県　加西　永長英夫≫

Please find attached our image of Jupiter this morning under fairly steady skies (finally....)
Note the prominence of BA and the intensity of the belts pr. and following this feature.
Very intense orange-red coloration within NEBzone which is very active in this span, as are both the
N and S components of the NEB.
Some very interesting demarcation along the NEBs seemingly strongly blue as noted in the Red image
attached.
[Dr. P. Clay Sherrod  Arkansas  State U.S.A]

2004/03/08 05:31, 05:41 UT
203 mm Newtonian: ToUcam Pro  Seeing 3-5/10 Trans 8/10
Here's my latest images of Jupiter from last night. Seeing was fair to good
(3-5/10).
[ Thomas E. Williamson Albuquerque, New Mexico, USA ]

[Bruno Daversin  Cherbourg, France]

Here are the aligned IR+CH4 pairs obtained on Mar08. More methane and IR
images will follow when possible. SEB disturbance is seen. Please notice the
IR-CH4 mismatches in SEB, some methane negative rifts in NEB, and some
methane positivity on IR bright clouds of the SEB disturbance (on other SEB
regions the most frequent observation is methane positivity colocalizing
with IR-dark material).


Here are some broadband images obtained on 08 Mar, showing the SEB
disturbance. Arrowed in an inset is a bright EZ cloud that may be preceding
the EZs slightly bluish (when near the limb) feature that has been described
earlier by other observers. Is this possible?
≪アントニオ  シダダオ  ポルトガル≫
[Antonio Cidadao  Oeiras - Portugal]

[Damian Peach: Loudwater, Buckinghamshire, UK.]

ALPO-Japan Latest Jupiter Section