Kutup \u0131\u015f\u0131klar\u0131, ya da aurora, genellikle kutup b\u00f6lgelerinde g\u00f6r\u00fclen bir gece \u0131\u015f\u0131mas\u0131d\u0131r. Aurora, g\u00f6ky\u00fcz\u00fcndeki do\u011fal \u0131\u015f\u0131k g\u00f6r\u00fcnt\u00fcleridir. Genelde gece g\u00f6r\u00fclen aurora, \u00e7\u0131plak g\u00f6zle de izlenebilir. Kuzey Yar\u0131k\u00fcredeki aurora g\u00f6r\u00fcnt\u00fcs\u00fcne aurora borealis, G\u00fcney Yarik\u00fcre\u2019dekine de aurora australis denir. Auroralar, g\u00fcne\u015fin d\u00fcnya atmosferi \u00fczerindeki etkilerinin en belirgin \u015fekilde g\u00f6r\u00fclebilenidir.<\/p>\n
\u00c7o\u011fu auroralar y\u00fcksek kuzey ve g\u00fcney enlemlerinde g\u00f6r\u00fcl\u00fcr. \u00d6zellikle yay, bulut ve \u00e7izgi \u015feklinde olu\u015furlar. Baz\u0131lar\u0131 hareket eder, parlakla\u015f\u0131r ya da aniden yan\u0131p s\u00f6nerler. Ye\u015fil, auroralarin en yayg\u0131n rengidir. Ancak \u00e7ok y\u00fckseklerde olan auroralar k\u0131rm\u0131z\u0131 ya da pembe olabilirler. \u00c7o\u011fu aurora atmosferin 100 ile 1000 km aral\u0131\u011f\u0131nda olu\u015fur. Baz\u0131lar\u0131 atmosfer boyunca binlerce kilometre yatay uzunlu\u011fa sahip olabilir.<\/p>\n
Aurora g\u00f6r\u00fcnt\u00fcleri, g\u00fcne\u015ften gelen solar r\u00fczgarlardaki y\u00fckl\u00fc par\u00e7ac\u0131klar\u0131n atmosferle etkile\u015fmesi sonucu olu\u015fur. Bu par\u00e7ac\u0131klar d\u00fcnyan\u0131n manyetik alan\u0131na ula\u015ft\u0131\u011f\u0131nda baz\u0131lar\u0131 kap\u0131l\u0131r. Bu par\u00e7alar\u0131n \u00e7o\u011fu d\u00fcnyan\u0131n manyetik kutuplar\u0131na \u00e7ekilirler. Bu par\u00e7ac\u0131klar atmosferdeki molek\u00fcllerle \u00e7arp\u0131\u015ft\u0131klar\u0131nda enerji a\u00e7\u0131\u011fa \u00e7\u0131kar. Bu enerjinin bir k\u0131sm\u0131 da auroralar \u015feklinde sal\u0131n\u0131r.<\/p>\n
Auroralar s\u0131kl\u0131kla 11 y\u0131ll\u0131k g\u00fcne\u015f d\u00f6ng\u00fcs\u00fcn\u00fcn en yo\u011fun zaman\u0131nda g\u00f6r\u00fcl\u00fcr. Bu d\u00f6nemde, g\u00fcne\u015f y\u00fczeyindeki koyu lekeler say\u0131ca artar. G\u00fcne\u015fteki \u015fiddetli patlamalar g\u00fcne\u015f lekeleriyle ilgilidir. Solar patlamalardan \u00e7\u0131kan elektronlar ve protonlar, d\u00fcnya atmosferiyle etkile\u015fir. Bu etkile\u015fim olduk\u00e7a parlak auroralar yarat\u0131r. Bu ayn\u0131 zamanda d\u00fcnyan\u0131n manyetik alan\u0131nda g\u00fc\u00e7l\u00fc dalgalanmalar meydana getirir; (manyetik f\u0131rt\u0131na). Bu f\u0131rt\u0131nalar esnas\u0131nda auroralar kutup b\u00f6lgelerinden ekvatora do\u011fru kayar.<\/p>\n","protected":false},"excerpt":{"rendered":"
Kutup \u0131\u015f\u0131klar\u0131, ya da aurora, genellikle kutup b\u00f6lgelerinde g\u00f6r\u00fclen bir gece \u0131\u015f\u0131mas\u0131d\u0131r. Aurora, g\u00f6ky\u00fcz\u00fcndeki do\u011fal \u0131\u015f\u0131k g\u00f6r\u00fcnt\u00fcleridir. Genelde gece g\u00f6r\u00fclen aurora, \u00e7\u0131plak g\u00f6zle de izlenebilir. Kuzey Yar\u0131k\u00fcredeki aurora g\u00f6r\u00fcnt\u00fcs\u00fcne aurora borealis, G\u00fcney Yarik\u00fcre\u2019dekine de aurora australis denir. Auroralar, g\u00fcne\u015fin d\u00fcnya atmosferi \u00fczerindeki etkilerinin en belirgin \u015fekilde g\u00f6r\u00fclebilenidir. \u00c7o\u011fu auroralar y\u00fcksek kuzey ve g\u00fcney enlemlerinde g\u00f6r\u00fcl\u00fcr. …<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[1407,1403],"tags":[2796,2134,2730,6725,6726,2138],"class_list":["post-2714","post","type-post","status-publish","format-standard","hentry","category-fen-ve-teknoloji-odevleri","category-odevler","tag-atmosfer","tag-elektron","tag-gunes","tag-kutup-isiklari","tag-manyetik-firtina","tag-proton"],"_links":{"self":[{"href":"https:\/\/www.islamidavet.com\/kutuphane\/wp-json\/wp\/v2\/posts\/2714","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.islamidavet.com\/kutuphane\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.islamidavet.com\/kutuphane\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.islamidavet.com\/kutuphane\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/www.islamidavet.com\/kutuphane\/wp-json\/wp\/v2\/comments?post=2714"}],"version-history":[{"count":0,"href":"https:\/\/www.islamidavet.com\/kutuphane\/wp-json\/wp\/v2\/posts\/2714\/revisions"}],"wp:attachment":[{"href":"https:\/\/www.islamidavet.com\/kutuphane\/wp-json\/wp\/v2\/media?parent=2714"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.islamidavet.com\/kutuphane\/wp-json\/wp\/v2\/categories?post=2714"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.islamidavet.com\/kutuphane\/wp-json\/wp\/v2\/tags?post=2714"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}