火星 ALPO-Japan Latest
Mars Image 2018/10/10(UT)
佐藤康明
Christopher Go,Javier Beltran Jovani,Paul Maxson,Joaquin Camarena,Milika-Nicholas
Christopher Go,Javier,P.Maxson,Y.Sato,J.Camarena,Milika-Nicholas
解説（安達）/ Comment by Makoto Adachi
Milika-Nicholas氏の緑画像では、北極の周辺に濃いダストのベールが記録されている。この画像を見ると、Alcyoniusの暗斑や
Aetheriaの暗斑も記録されておらず、この付近の北半球全体がダスティーであることが分かる。また、同じようにEridaniaの南方まで
広がったダストストームは、ＳＰＣの縁にまで広がっている様子が記録されている。
In the green image of Mr. Milika-Nicholas, a veil of dense dust is recorded around the North Pole. Looking at this image, neither
dark spots of Alcyonius nor dark spots of Aetheria are recorded, and it is understood that the entire northern hemisphere around this is dusty.
Similarly, the dust storm spreading to the south of Eridania is recorded to the edge of the SPC.
（by 6 observations ;reported by Makoto Adachi)
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We had some good conditions today.
Surprisingly,here are no tropical systems on the West Pacific region.
Seeing was good today.
These images show Syrtis Major. Hellas is clear of clouds!
Hellas happens to be the largest VISIBLE impact basin in the Solar System.
Mare Tyrrhenum and Syrtis Minor are well resolved.
The Mitchel Mountains can be seen detached from the south pole.
[Christopher Go : Cebu Philippines]
[Javier Beltran Jovani:Castellon-Spain]
[ Paul Maxson:Surprise,Arizona,United States]
薄曇りの状態で撮りました。極冠が非常に小さくなりましたね。
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[Sagamihara-shi Kanagawa-prefecture Japan]
≪神奈川県相模原市 佐藤康明≫
[Joaquin Camarena:Spain]
Poor seeing but very fast fps & single channel capture durations of 140 seconds each helped with the amount of frame numbers to work with. Hellas appeared very bright in all channels: the r-g-b images and single channels are about 2.5 hours apart with Syrtis Major in full view by the later capture. Also included are 4 captures with iR filters - 3 in 610nm & one in 685nm.
[Milika-Nicholas:Adelaide,South Australia]
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