土星 ALPO-Japan Latest
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Saturn Image 2015/05/13(UT)
熊森照明
Trevor Barry,Constantin Sprianu,Milika-Nicholas
T.Barry,T.Kumamori,C.Sprianu,Milika-Nicholas
Trevor Barry(406mm Newtonian) |
Imaged Saturn May 13th,seeing was effected by the jet stream to various degrees but have a few data sets from the session.
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[Trevor Barry:Broken Hill:Australia]
Teruaki Kumamori (280mm SC) |
台風一過の青空でしたが、シーイングは良くありません
≪大阪府堺市 熊森照明≫[Teruaki Kumamori:Ohsaka Japan]
Constantin Sprianu(245mm Cassegrain) |
This is Saturn in average seeing and (very) low altitude (26 degrees).
Even with the ADC is hard to make good images without very good seeing.
Seeing 5/10,Transparency 8/10
[Constantin Sprianu:Otopeni,Romania]
Milika-Nicholas (355mm SCT) |
We noted what we termed a large "rift" or "disturbance" in one of Saturn's
Northern bands in the area from 60°N to 67°N at L1 = 183° L2 = 260° L3 =
266° (approximate) in these images.
Although we do not think that it had been reported upon before (we notified
BAA & PVOL) we then examined ALPO images from other contributors from
earlier dates & were able to ascertain that this feature had been in
existence for some time, albeit slightly different in appearance & often
somewhat obscure...some imagers referring to it as a "dark spot."
At the time it appeared like a "notch" in the darker more northerly
band/belt adjacent to the lighter more southerly band/belt ( which we
interpret as the NNTeZ & NNTeB)
The iR742nm images displays the greatest contrast as would be expected
although the r & r animation as well as the rgb define it better for that
particular date.
Subsequent images show this feature evolving rapidly & changing in
appearance to what looks like a dark spot with a proceeding longitudinal
disturbance or "wake."
[Milika-Nicholas:Adelaide,South Australia]