Avtory i prava: Olivier Staiger
Poyasnenie:
Lunnye
zatmeniya proishodyat dostatochno medlenno, i my mozhem
nablyudat' ih ne toropyas'.
Ih mogut videt' vse na nochnoi
storone Zemli
pri horoshih pogodnyh usloviyah, pri etom polnaya faza
zatmeniya chasto dlitsya poryadka chasa, poka
luna prohodit cherez zemnuyu ten'.
Chto kasaetsya solnechnyh
zatmenii , to oni gorazdo bolee bystrotechnye.
Polnaya faza prodolzhaetsya neskol'ko minut, a uvidet' ih mogut
tol'ko te schastlivchiki, kotorye okazhutsya v oblasti prohozhdeniya
lunnoi teni po poverhnosti Zemli.
Vo vremya kol'cevogo solnechnogo zatmeniya 29 aprelya 1995 goda
fotograf Olivier
Staiger nahodilsya v Ekvadore (Makara). Nebo bylo chastichno
zatyanuto oblakami.
Emu udalos' poluchit' etot snimok, na kotorom vozle Solnca
vidna letyashaya ptica, neposredstvenno pered fazoi maksimuma
kol'cevogo zatmeniya.
Sleduyushee solnechnoe zatmenie, kotoroe proizoidet
10 iyunya, takzhe budet kol'cevym.
Chastnye fazy zatmeniya budut
vidny iz vostochnoi Azii, s
Tihogo Okeana i s bol'shei chasti Severnoi
Ameriki.
Momenty
zatmenii rasschitany zaranee i izvestny s bol'shoi
tochnost'yu.
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NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.
Publikacii s klyuchevymi slovami:
solar eclipse - eclipse - annular solar eclipse - Solnechnoe zatmenie - kol'cevoe zatmenie - chastnoe solnechnoe zatmenie
Publikacii so slovami: solar eclipse - eclipse - annular solar eclipse - Solnechnoe zatmenie - kol'cevoe zatmenie - chastnoe solnechnoe zatmenie | |
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