Poyasnenie: V vidimom spektre Solnca vo vremya korotkoi polnoi fazy zatmeniya 3-go noyabrya linii poglosheniya prevratilis' v emissionnye linii. Etot korotkii moment udalos' zapechatlet' s pomosh'yu teleob'ektiva i difrakcionnoi reshetki na izobrazhenii, poluchennom pri proyasnyayushemsya nebe nad Gabonom v ekvatorial'noi Afrike. Kogda svet ot solnechnogo diska zakryt Lunoi, obychno dominiruyushii absorbcionnyi spektr solnechnoi fotosfery takzhe skryt. Ostavsheesya svechenie razlozheno difrakcionnoi reshetkoi v spektr, kotoryi viden sprava ot Solnca. Eto – otdel'nye izobrazheniya zatmeniya na raznyh dlinah voln, izluchaemyh atomami vdol' uzkoi dugi solnechnoi hromosfery. Samye yarkie izobrazheniya, ili samye sil'nye hromosfernye emissionnye linii dayut atomy vodoroda. Oni sozdayut krasnuyu emissiyu Hα okolo pravogo kraya spektra i golubuyu liniyu Hβ sleva. Yarkaya zheltaya emissiya v seredine sozdaetsya atomami geliya – elementa, kotoryi byl otkryt v spektre vspyshki Solnca.

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Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (USRA)
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Publikacii s klyuchevymi slovami: spectrum - solar eclipse - Solnechnoe zatmenie - Spektr Publikacii so slovami: spectrum - solar eclipse - Solnechnoe zatmenie - Spektr
Sm. takzhe: Zatmenie na voshode Solnce i propavshie cveta Solnechnoe zatmenie s korablya Solnechnoe zatmenie v Zapadnoi Avstralii Vostorzhennoe solnechnoe zatmenie Solnechnoe zatmenie i bumazhnaya Luna Zatmenie na vode Vse publikacii na tu zhe temu >>