\n<\/p>\n
“GER\u00c7EK B\u0130R OYUN DE\u011e\u0130\u015eT\u0130R\u0130C\u0130”<\/p>\n
\u00a0<\/p>\n
W\u00f6ger, g\u00fcne\u015f KHI’sinin ke\u015ffini “ger\u00e7ek bir oyun de\u011fi\u015ftirici” olarak niteledi ve bunun G\u00fcne\u015f’in kendi atmosferine nas\u0131l enerji sa\u011flad\u0131\u011f\u0131n\u0131 anlamak i\u00e7in yeni bir \u00e7er\u00e7eve a\u00e7t\u0131\u011f\u0131n\u0131 s\u00f6yledi.<\/p>\n
\u00a0<\/p>\n
Ulusal G\u00fcne\u015f G\u00f6zlemevi g\u00f6kbilimcisi ve \u00e7al\u0131\u015fman\u0131n e\u015f ba\u015fyazar\u0131 David Kuridze, “G\u00fcne\u015f ve G\u00fcne\u015f benzeri y\u0131ld\u0131zlar, manyetik unsurlar\u0131 i\u00e7inde h\u0131zl\u0131 ve patlamal\u0131 olaylardan olu\u015fan b\u00fct\u00fcn bir spektrumla karakterize edilen son derece dinamik sistemlerdir. Bu patlamalar\u0131n nas\u0131l tetiklendi\u011fi, modern g\u00fcne\u015f fizi\u011findeki ana s\u0131n\u0131rlardan biridir” dedi.<\/p>\n
\u00a0<\/p>\n
KHI tezah\u00fcr\u00fc, G\u00fcne\u015f’in d\u0131\u015f atmosferinin neden bu kadar \u0131s\u0131nd\u0131\u011f\u0131n\u0131 ve manyetik enerjinin G\u00fcne\u015f y\u00fczeyinde neden birikti\u011fini ve hareket etti\u011fini a\u00e7\u0131klamaya yard\u0131mc\u0131 olabilir.<\/p>\n
\u00a0<\/p>\n
Kuridze, KHI taraf\u0131ndan \u00fcretilen s\u00fcrekli b\u00fck\u00fclme hareketlerinin, ta\u00e7k\u00fcre k\u00fctle at\u0131mlar\u0131n\u0131 ve g\u00fcne\u015f patlamalar\u0131n\u0131 tetiklemek i\u00e7in gereken enerjiyi kademeli olarak in\u015fa edebilece\u011fini s\u00f6yledi.<\/p>\n
\u00a0<\/p>\n
Ta\u00e7k\u00fcre k\u00fctle at\u0131mlar\u0131, G\u00fcne\u015f y\u00fczeyinden f\u0131rlat\u0131lan ve manyetik alan \u00e7izgileriyle \u00f6r\u00fclm\u00fc\u015f devasa gaz kabarc\u0131klar\u0131n\u0131 ifade ediyor. G\u00fcne\u015f patlamalar\u0131 ise \u0131\u015f\u0131\u011f\u0131, enerjiyi ve y\u00fcksek h\u0131zl\u0131 par\u00e7ac\u0131klar\u0131 uzaya savuran G\u00fcne\u015f \u00fczerindeki devasa patlamalar.<\/p>\n<\/div>\n