Avtory i prava: Hans Coeckelberghs
Poyasnenie:
Esli vidimyi
diametr Luny okazhetsya
men'she vidimogo diametra Solnca vo vremya
solnechnogo zatmeniya, zatmenie budet
kol'cevym,
i my uvidim siluet Luny v okruzhenii "ognennogo kol'ca" solnechnogo sveta.
Imenno takoe zrelishe mozhno bylo
nablyudat' 31 maya v vysokih shirotah
severnogo polushariya, kogda vo vremya novoluniya
lunnyi disk prohodil
po solnechnomu disku.
Etot den' okazalsya ne ochen' udachnym dlya
lyubitelei
astronomii, raspolozhivshihsya na myse Rat (Cape Wrath) na severo-zapadnom poberezh'e
Shotlandii. Nebo na vostoke v den' zatmeniya bylo zatyanuto oblakami.
K schast'yu, za neskol'ko minut do kol'cevoi fazy Solnce vyshlo iz-za tuch, i
astronomu Gansu Kekel'bergsu, kotoryi reshil zhdat' do konca, nakonec povezlo:
on sumel s pomosh'yu teleskopa sdelat' snimok
zatmeniya Solnca.
Na snimke ognennoe kol'co prosvechivaet skvoz' krasnovatyi oblachnyi sloi.
V yuzhnom polusharii v etom godu tozhe ne oboidetsya bez zatmeniya:
23 noyabrya proizoidet sleduyushee solnechnoe zatmenie. Ego polnaya faza
budet vidna vdol' polosy, kotoraya protyanetsya cherez Antarktiku.
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NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.
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Publikacii s klyuchevymi slovami:
solar eclipse - annular solar eclipse - Scotland - Solnechnoe zatmenie - kol'cevoe zatmenie
Publikacii so slovami: solar eclipse - annular solar eclipse - Scotland - Solnechnoe zatmenie - kol'cevoe zatmenie | |
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