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Jupiter Image 2021/07/01(UT)
Vlamir da Silva Junior,Guan.Zhong Wang,Javier Beltran Jovani,Gerald Stelmack,Manolo Rodriguez,Paulo Casquinha
V.da Silva Jr.,G.Z.Wang,Javier,G.Stelmack,M.Rodriguez,P.Casquinha
This was the time of Oval BA,close at the CM in the IR742 image and presenting something in the center of it,
which I can not resolve without this filter.
I'm really glad with the good result I got on the area following NN-WS6 with this filter,
a lot of dark spots following it.
NTBn is showing its wavy like structure on the preceding side.
Note the SEBs rings appearing as some grayish long features.
The SSTB ovals area also present,specilly the one just south of Oval BA.
WS6 (the spot preceding Oval BA) is brighter than Oval BA.
[Vlamir da Silva Junior : Sao Paulo,Brazil]
[Guan.Zhong Wang : Taichung,Taiwan]
[Javier Beltran Jovani:Castellon-Spain]
[G.Stelmack : Canada]
Average conditions of seeing 3/5 estimate,good transparency 4/5
Acceptable conditions of seeing 3.5/5 estimate,good transparency 4/5
Numerous surface details are very evident,highlighting the Oval BA near the eastern limb of the STB,
the small white storms A1 to A5 of the SSTB and the WSZ in the NTB,as well as the rifled region in the NEBn
[Manolo Rodriguez : El Pedroso,Seville,Spain]
(site: 38.567 N /8.933 W Alt 124 m)
[Paulo Casquinha Palmela,Portugal]
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