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Saturn Image 2025/11/02(UT)
皆川伸也,高松 泉,森田光治
Manos Kardasis,Vicent Gonzalez Cebria,Paul G. Abel
N.Minagawa,Kardasis,I.Takamatsu,M.Morita,V.Gonzalez,P.Abel
19時から1時間程度シーイングが良好でした。
≪東京都 立川市 皆川伸也≫[Nobuya Minagawa:Tokyo Japan]
in good conditions among clouds here are some sets:
[Manos Kardasis,Glyfada-Athens;Greece]
《カーダシス マノス:ギリシャ アテネ》
≪高松 泉 : ≫[Izumi Takamatsu: Arakawa,Tokyo,Japan]
南中付近でやや改善したものの気流が不安定で満足なシーイングではなかった。
≪滋賀県守山市 森田光治≫[Mitsuji Morita:Siga Japan]
[Vicent Gonzalez Cebria:46600 Alzira(Valencia) Spain]
in average seeing conditions. The rings are now just -0.6° open and look like a slither of light. Although conditions were average and a power of x230 could only be used, a number of points of interest were observed:
The Globe:
・SPR: A vague greyish region with very little detail observed
・SSTB-STB: Both belts seen but the SSTB quite faint, both a brownish colour and the regions around contained a subtle greenish tint.
・SEB: A broad belt- for the first time I was able to see a darker southern SEB(s) component. The SEB(N) was quite prominent and seemd to be fairly smooth tonight.
・EZ: A bright zone with a thin grey EB seen in both regions. The SHRG were visible north of the rings.
・NEB: A broad belt with two components- the NEB(s) was the darker of the two and again fairly uniform.
・NNTB-N3TB: Two thin belts, bluish in colour. The S3TB was the darker of the two.
・NPR: A vague greyish region.
The Rings: A very thin line now, they appeared uniform although a vague greyish patch could be seen where the Cassini Division would be. The rings appeared to have a brownish tint. The satellite Rhea could be seen and this also had a warm tone to it. By 2008UT the seeing dropped off and observations were concluded for the night.
[Paul G. Abel:Leicester:United Kingdom]
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