木星 月惑星研究会 関西支部 （最新）


ALPO-Japan Latest
Jupiter Image 2004/01/06(UT)

福井英人,大田 聡,堀川邦昭,
Fattinnanzi Cristia,Paulo Casquinha,Antonio Cidadao

H.Fukui,S.Ota,K.Horikawa,C.Fattinnanzi,P.Casquinha,A.Cidadao

Hideto Fukui (250mm Dall Kirkham, Philips ToUcam Pro) 
[Hideto.Fukui  (Kyoto City  Japan)]
≪京都府  京都市  福井英人≫

Satoshi Ota (319mm Newtonian, Qcam pro4000) 
[Tomigusuku city Okinawa Japan]
≪沖縄県  豊見城市  大田 聡≫

Kuniaki Horikawa(160mm Newtonian, Drawing & ToUcam PRO) 
[Horikawa_J20040106-1624_drw.jpg]
2004/01/06 16h24m(UT)
I=215.1 II=164.5
Seeing=6-7/10 Transparency=1-3/5
16cm Refl. x200
・mid-SEB outbreak後端は明瞭
・BAは周囲が薄暗く捉えやすいが、透明度低下のためCMTは取れなかった



[Horikawa_J20040106-1747_img.jpg]
2004/01/06 17h47m(UT)
I=265.8 II=214.6 De=-1.7 Dia=40.3
Seeing=6/10 Transparency=1/5
16cm Refl. x143
Philips ToUcam Pro 465 frames composite
≪神奈川県横浜市泉区  堀川邦昭≫

Fattinnanzi Cristian ( 250mm Newtonian Philips Vesta Pro) 

[Fattinnanzi Cristian :  Macerata ITALY]
Paulo Casquinha ( 200mm f/5 Newton Reflector Toucam Pro)

(site: 38.567 N /8.933 W Alt 124 m)
[Paulo Casquinha Palmela, Portugal]
Antonio Cidadao (250mm LX200SCT : FLICM7 1E CCD camera) 
Here is Jan6 data, obtained under a bit better seeing.
Notice that the SSTB methane-bright area just following the GRS corresponts
to the diffuse oval between the two smal spots visible in broadband IR and
not to the spots themselves.
Also notice that I include IR data from two filters (700 and 830nm). As for
the Saturn globe, these filters produce different results, and those having
them may find interesting to make image ratios from registered images. In
jupiter, for instance, the higher latitudes are considerably darker in the
raws.




Here is the jan06 methane time-lapse animation produced by the bias, dark
and flat corrected raws of the processed images previously sent.

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