火星 ALPO-Japan Latest

Mars Image 2014/05/10(UT)
米山誠一,松本博久,三品利郎,池村俊彦,菅野清一,畑中明利,熊森照明,瀧本郁夫,尾崎公一,永長英夫
Stanislas Maksmowicz,Gerald Stelmack,Carmelo Mel Zannelli,Bruce Macdonald,Manos Kardasis
S.Yoneyama,H.Matsumoto,T.Mishina,T.Ikemura,S.Kanno,A.Hatanaka,T.Kumamori,I.Takimoto,S.Maksmowicz,G.Stelmack,C.Zannelli,B.Macdonald,K.Ozaki,Kardasis,H.Einaga

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今夜もシーイングの変化が激しい状態でした。

≪神奈川県横浜市  米山誠一≫[Seiichi Yoneyama:Kanagawa Japan]

seeing 4〜5/10 trans 5/5
昨晩よりシーイングは良くなり、最近撮影した中では一番条件が良かったと
思います。
Orion30cmF5.3  Kasai Trading 3Elements 2X Barlow Lens + 64mm Extension Tube  (F25)
Takahashi NJP    ASI120MC  Planetary Atmospheric Dispersion Corrector
Colour image:  6ms  167fps  2000/20000 frames stacked  320X240 Gain100  Gamma1
（ Resize  180％ )

[Hirohisa.Matsumoto  (Kurayoshi City Tottori-Prefecture Japan)]
≪鳥取県 倉吉市　松本博久≫

≪神奈川県  横浜市  三品利郎≫[Toshirou.Mishina:Kanagawa Japan]

[T.Ikemura Nagoya Aichi JAPAN]
≪愛知県名古屋市  池村俊彦≫

相変わらずシーイングは良くありません。

≪山形県上山市  菅野清一≫[Seiichi Kanno:Yamagata Japan]

≪三重県熊野市  畑中明利≫[Akitoshi Hatanaka:Kumano Mie Japan]

北極冠近くの雲は拡散したみたいですね。

≪大阪府堺市 熊森照明≫[Teruaki Kumamori:Ohsaka Japan]

約1.5時間火星を見ていたが、縁が絶えずボケているようで、撮影後半は、ピントが
どこで合っているか判らないほどとなった。


[Ayauta-gun Kagawa-Prefecture Japan]
≪香川県  綾歌郡  瀧本郁夫≫

I followed Mars almost narrowly since 27-28 April,3rd May and 7-8-9_10th
May. The 3rd May report showed deep yellowish disk with faded contrast of
features. At the 27-28th April,feature contrasts were conspiscious for
main ones on a similar portion of Mars.
However,it should be interresting to remind some facts about the
reflectivity noted on some "white" clouds catched at limbs,especially on
the Syrtis Major occulted by.
S.M. was occulted by white hazze and and dust aswell,therefore by mist.
S.M. was not visible by these dense hazze in all colors when just escaping
the limb.
At the opposite limb the situation was on a similar figure.
On 27-28 April,presence of mist rather than pure white-blue clouds at
limbs. Dust was at a density not negligeable already,but the overall disk
color was not what we saw on the 3rd May.
So dust storm on the 30th April near the cap,well ok,but this is adding
on the density in atmosphere for the least.
We should have a threeshold of dust density to reach in already white hazzy
atmosphere for changing the discoloring of the disk. There should have also
a saturation phenomena for creating this dense mist.
Yesterday the 10th May at the 100mm refractor,it appear to me that the
discoloration is fading and the contrasts levels of features on the
temperate zones are enhanced,but planet color under naked eyes was still
yellowish.
May be the beginning of the atmosphere clearing from dust.
Ididn't have the time and the opportunity to push the violet filter because
of the presence of sky clouds here.
We will see the development of this event later as it will become.

[Stanislas Maksymowicz  Ecquevilly,France]

C9.25 SCT @ f33
DMK21AF04.AS
Astronomik LRGB Type 2 Filter Set
2014/05/10 04:49 UT
CM = 228.11
Mag = -0.97
Dia = 13.81"
Phase = 0.95

[G.Stelmack : Canada]

[Carmelo Mel Zannelli,Sicily-Italy]

(Bruce Macdonald : Punta Gorda,Florida USA)

[Ki.Ozaki,Sobue Inazawa Aichi JAPAN]
≪愛知県稲沢市祖父江町  尾崎公一≫

poor to average seeing.
Southern haze especially in Icaria & Deuteronilus.
Clouds  around Olympus.Also from Boreum to Tempe up to Lunae Lacus.
Chasma Borealis is visible.Also some small isolated NPC remanents south of the main NPC body.

[Manos Kardasis,Glyfada-Athens;Greece]
《カーダシス マノス:ギリシャ アテネ》

[Hideo Einaga Kasai-City Hyogo-Prefecture Japan]
≪兵庫県  加西  永長英夫≫

ALPO-Japan Latest Mars Section	2014/05/11
	2014/05/09