2002/03/28 09:48:59 (UT)
CMI = 167.7, CMII =  31.1, CMIII = 130.1
De =  +1.9, E.Dia = 38.46"

7 frames composite
Seeing=5/10,Trans=3/5
25cm+barlow3x(F=34)+Picona(1/7s)

2002/03/28 10:22:48 (UT)
CMI = 188.3, CMII =  51.6, CMIII = 150.5
De =  +1.9, E.Dia = 38.45"

8 frames composite
Seeing=5/10,Trans=3/5
25cm+barlow3x(F=34)+Picona(1/7s)

2002/03/28 11:25:26 (UT)
CMI = 226.5, CMII =  89.4, CMIII = 188.4
De =  +1.9, E.Dia = 38.45"

7 frames composite
Seeing=3/10,Trans=2/5
25cm+barlow3x(F=34)+Picona(1/7s)

・BAはまだ消滅していないように思えるのですが‥。

HIDEO EINAGA ≪兵庫・加西　永長英夫≫

    2002/03/28 11:46:52(UT)
    �T=239.1  �U= 101.9  �V= 200.9
     De=+2.04  E.Dia= 38.68"
     25 Frames Composite

    2002/03/28  12:39:47(UT)
   �T=271.4  �U= 133.9  �V= 232.9
     De=+2.04  E.Dia= 38.68"
     23 Frames Composite

    seeing  4~6  /10

     40cm Cassegrain (F15)
     Or 25mm  Collimate
     2 degree Prizum
     SONY TRV-9  Video Camera

    seeing は、あまり良くないが、
　　時々良い瞬間がある。
　　ビデオ画像では、眼視よりぼやける事が
    多かったが、やはり良い瞬間があった。
≪三重県熊野市　畑中明利≫

Jupiter on Mar.28, 2002

[1]
2002/03/28 20:01:15 (JST)
2002/03/28 11:01:15 (UT)
CMI = 211.8, CMII =  74.8, CMIII = 173.8
28 frames composite

[3]
2002/03/28 20:22:53 (JST)
2002/03/28 11:22:53 (UT)
CMI = 225.0, CMII =  87.9, CMIII = 186.8
30 frames composite

Email:zba03198@bird.zero.ad.jp
Obs.site : Mozuhonmachi Sakai-City Osaka Japan
Telescope : C11 (SC) D=280mm fl=2800mm

Camera:Minolta DiMAGE5 (w/Minolta GT lens f=50.8mm)

Filter: IR Rejection built in the camera
Exposure : 0.07 sec
Effective F No.: 20 (XP24 mm relay lens)

Seeing = 7/10
Transparency = 3/6

Image Processing;
Software binning
Maximum Entropy Deconvolution
Enhanced with unsharp masking method.


ＢＥは健在です。ただし、シーイングが悪いと、
写りにくくなってしまいます。

ＤｉＭＡＧＥ５は、
たった、１０分間で１０００コマ近く撮れますので、
後の処理（というか選別が）が大変です。

　　　　　　≪大阪府　堺市　新川勝仁≫

 ≪栃木県　阿久津富夫≫




        

        Damian Peach (12" (30.5cm) Meade SCT @ f/21.0. ST-5c camera)
        
Hi all,
I am re sending the March 28th images, as there were errors in my first send.
The time and CM were incorrect, and there were registration artefacts present.
I attach the re-labled/processed image.
My apologies for the errors - it was late and i wanted to get the data out asap.
I will send additonal data from last night later.
Best Wishes

Hi all,

Here is the best set obtained on March 28th, before the ovals were visible.
Seeing was fairly favourable for these images. Of particular note is the dark
spot in the STrZ.

Best Wishes

Damian






*******************************************************************
Damian Peach. ALPO/BAA Jupiter Sections.
                            BAA Saturn Section.
E-mail: dpeach78@netscapeonline.co.uk
Homepage: http://www.the-planets.co.uk/
*******************************************************************
BAA Saturn Section:
http://members.netscapeonline.co.uk/dpeach78/index.htm
BAA Jupiter Section:
http://www.the-planets.co.uk/jupitersection/index.htm
*******************************************************************
[Rochester, Kent, UK.]
 ≪ダミアン−ピーチ　イギリス≫






        

        Antonio Cidadao (280mm C11+ST-237 CCD camera)
        











Here are some of the images obtained tonight in moments of good seeing.
More will follow tomorrow.

The merged SSTC oval looks slightly elongated and tilted (Sf. to Np.),
mostly in R, IR and clear filter. It continues to be followed by the new
(cyclonic) oval described by John on his message.

BA is very distinct with good seeing and shows internal structure (same
morphology in CH4 as in previous dates; images to follow).

All for now

Good observations

Antonio

Hi again,

When comparing this red image obtained tonight with the great Ed's images
grabbed earlier in Mar28, we can perhaps see some evidence of ccw rotation
on the merged spot.

Best

Antonio
 ≪アントニオ　シダダオ　ポルトガル≫
[Antonio Cidadao  Oeiras - Portugal ]




ALPO-Japan Latest　Jupiter Section