{"id":86656,"date":"2024-10-16T15:12:07","date_gmt":"2024-10-16T15:12:07","guid":{"rendered":"https:\/\/ekamu.net\/?p=86656"},"modified":"2024-10-16T15:12:07","modified_gmt":"2024-10-16T15:12:07","slug":"gunes-solar-maksimum-seviyesine-yukseldi-neler-yasanacak","status":"publish","type":"post","link":"https:\/\/ekamu.net\/index.php\/2024\/10\/16\/gunes-solar-maksimum-seviyesine-yukseldi-neler-yasanacak\/","title":{"rendered":"G\u00fcne\u015f, \u201csolar maksimum\u201d seviyesine y\u00fckseldi: Neler ya\u015fanacak?"},"content":{"rendered":"

<\/span> NASA<\/strong> ve NOAA<\/strong> (Ulusal Okyanus ve Atmosfer Dairesi) yapt\u0131\u011f\u0131 a\u00e7\u0131klamaya g\u00f6re, G\u00fcne\u015f<\/strong>, 11 y\u0131ll\u0131k do\u011fal d\u00f6ng\u00fcs\u00fcnde “g\u00fcne\u015f maksimumu” veya \u201csolar maksimum<\/strong>\u201d olarak bilinen aktif d\u00f6neme ula\u015ft\u0131. Bu d\u00f6nemin \u00f6n\u00fcm\u00fczdeki y\u0131l boyunca devam edebilece\u011fi bildirildi.\u00a0NOAA, mevcut solar maksimumu s\u00fcresince daha fazla jeomanyetik f\u0131rt\u0131na ya\u015fanabilece\u011fini, bunun da \u00f6n\u00fcm\u00fczdeki aylarda Kuzey I\u015f\u0131klar\u0131\u2019n\u0131n (Aurora Borealis) daha s\u0131k g\u00f6r\u00fcnmesine neden olaca\u011f\u0131n\u0131 belirtti. <\/figure>\n

G\u00fcne\u015f, zirve d\u00f6nemine girdi<\/b><\/p>\n

G\u00fcne\u015f d\u00f6ng\u00fcs\u00fc, G\u00fcne\u015f’in manyetik aktivite seviyeleri aras\u0131nda ge\u00e7i\u015f yapt\u0131\u011f\u0131 do\u011fal bir s\u00fcre\u00e7<\/strong> konumunda. Yakla\u015f\u0131k her 11 y\u0131lda bir<\/strong>, bu d\u00f6ng\u00fcn\u00fcn en y\u00fcksek noktas\u0131nda G\u00fcne\u015f\u2019in manyetik kutuplar\u0131 tersine d\u00f6ner. Bu, D\u00fcnya’da her on y\u0131lda bir Kuzey ve G\u00fcney kutuplar\u0131n\u0131n yer de\u011fi\u015ftirmesi gibi bir durumu and\u0131r\u0131r. Bu s\u00fcre\u00e7te G\u00fcne\u015f, sakin ve stabil bir durumdan aktif ve f\u0131rt\u0131nal\u0131<\/strong> bir hale ge\u00e7i\u015f yap\u0131yor.<\/p>\n

NASA ve NOAA, G\u00fcne\u015f lekelerini takip ederek G\u00fcne\u015f d\u00f6ng\u00fcs\u00fcn\u00fcn ilerlemesini ve aktivite seviyelerini tahmin ediyor. G\u00fcne\u015f lekeleri, manyetik alanlar\u0131n yo\u011funla\u015ft\u0131\u011f\u0131, G\u00fcne\u015f\u2019in daha so\u011fuk b\u00f6lgeleridir ve bu alanlar, G\u00fcne\u015f y\u00fczeyinde g\u00f6r\u00fcnen aktif b\u00f6lgeleri temsil ediyor. Bu aktif b\u00f6lgeler, g\u00fcne\u015f patlamalar\u0131n\u0131n ve di\u011fer olaylar\u0131n kayna\u011f\u0131 olarak biliniyor.<\/p>\n

Solar maksimum<\/strong> s\u0131ras\u0131nda<\/strong> bu lekelerin say\u0131s\u0131 ve dolay\u0131s\u0131yla G\u00fcne\u015f\u2019teki aktivitelerin say\u0131s\u0131 art\u0131\u015f g\u00f6steriyor<\/strong>. Bu d\u00f6ng\u00fc, G\u00fcne\u015f hakk\u0131nda yeni bilgiler edinilmesi i\u00e7in g\u00fczel bir f\u0131rsat sunarken ayn\u0131 zamanda D\u00fcnya’da ve G\u00fcne\u015f Sistemi \u00fczerinde somut etkilere<\/strong> neden oluyor.<\/p>\n

D\u00fcnya \u00fczerindeki etkileri<\/b><\/p>\n

<\/span> G\u00fcne\u015f aktiviteleri, “uzay havas\u0131” olarak bilinen ko\u015fullar\u0131 etkiler ve bu da hem uzaydaki uydular\u0131<\/strong> ve astronotlar\u0131<\/strong> hem de D\u00fcnya\u2019daki ileti\u015fim<\/strong> ve navigasyon<\/strong> sistemlerini, radyo<\/strong> ve GPS sinyallerini<\/strong> etkileyebilir. Hatta elektrik \u015febekelerine<\/strong> dahi zarar verebilir. G\u00fcne\u015fin en aktif oldu\u011fu d\u00f6nemlerde, bu t\u00fcr uzay hava olaylar\u0131 daha s\u0131k meydana gelmekte. Hat\u0131rlanaca\u011f\u0131 gibi \u00f6zellikle son aylarda ya\u015fanan G\u00fcne\u015f aktiviteleri g\u00fc\u00e7l\u00fc aurora (kuzey \u0131\u015f\u0131klar\u0131) olu\u015fumlar\u0131na ve uydular \u00fczerinde etkili olan jeomanyetik f\u0131rt\u0131nalara yol a\u00e7m\u0131\u015ft\u0131. <\/figure>\n
<\/span> 2024 y\u0131l\u0131n\u0131n May\u0131s ay\u0131nda, b\u00fcy\u00fck G\u00fcne\u015f patlamalar\u0131 ve koronal-ta\u00e7k\u00fcre k\u00fctle at\u0131l\u0131mlar\u0131<\/strong> (CME) D\u00fcnya’ya do\u011fru manyetik alan ve y\u00fckl\u00fc par\u00e7ac\u0131klar\u0131 g\u00f6ndermi\u015fti. Bu olaylar, son 20 y\u0131l\u0131n en g\u00fc\u00e7l\u00fc jeomanyetik f\u0131rt\u0131nas\u0131n\u0131<\/strong> ve belki de son 500 y\u0131l\u0131n en etkileyici aurora g\u00f6r\u00fcnt\u00fclerini olu\u015fturmu\u015ftu. Son bir y\u0131ldaki aktivite art\u0131\u015f\u0131 nedeniyle kuzey \u0131\u015f\u0131klar\u0131 T\u00fcrkiye\u2019nin kuzey kesimlerinden bile g\u00f6r\u00fclm\u00fc\u015ft\u00fc. <\/figure>\n

Bununla birlikte NASA ve NOAA taraf\u0131ndan yap\u0131lan a\u00e7\u0131klama, G\u00fcne\u015f aktivitesinin zirve yapt\u0131\u011f\u0131 anlam\u0131na gelmiyor; sadece zirve d\u00f6nemine girdi\u011fimizi ifade ediyor. Aktivitelerin zirveye ula\u015ft\u0131\u011f\u0131 ay\u0131 belirlemek birka\u00e7 ay veya y\u0131l s\u00fcrebilir.<\/p>\n\n

<\/span><\/p>\n

Kaynak :\u00a0https:\/\/www.donanimhaber.com\/gunes-11-yillik-dongusunde-solar-maksimum-seviyesine-yukseldi–183150<\/span><\/p>\n","protected":false},"excerpt":{"rendered":"

NASA ve NOAA (Ulusal Okyanus ve Atmosfer Dairesi) yapt\u0131\u011f\u0131 a\u00e7\u0131klamaya g\u00f6re, G\u00fcne\u015f, 11 y\u0131ll\u0131k do\u011fal d\u00f6ng\u00fcs\u00fcnde “g\u00fcne\u015f maksimumu” veya \u201csolar maksimum\u201d olarak bilinen aktif d\u00f6neme ula\u015ft\u0131. Bu d\u00f6nemin \u00f6n\u00fcm\u00fczdeki y\u0131l boyunca devam edebilece\u011fi …<\/p>\n","protected":false},"author":1,"featured_media":86657,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[8],"tags":[235,5180,212,469,263],"class_list":["post-86656","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-teknoloji","tag-aktif","tag-aktivite","tag-dunya","tag-gunes","tag-kuzey"],"_links":{"self":[{"href":"https:\/\/ekamu.net\/index.php\/wp-json\/wp\/v2\/posts\/86656","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/ekamu.net\/index.php\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/ekamu.net\/index.php\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/ekamu.net\/index.php\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/ekamu.net\/index.php\/wp-json\/wp\/v2\/comments?post=86656"}],"version-history":[{"count":1,"href":"https:\/\/ekamu.net\/index.php\/wp-json\/wp\/v2\/posts\/86656\/revisions"}],"predecessor-version":[{"id":86661,"href":"https:\/\/ekamu.net\/index.php\/wp-json\/wp\/v2\/posts\/86656\/revisions\/86661"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/ekamu.net\/index.php\/wp-json\/wp\/v2\/media\/86657"}],"wp:attachment":[{"href":"https:\/\/ekamu.net\/index.php\/wp-json\/wp\/v2\/media?parent=86656"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/ekamu.net\/index.php\/wp-json\/wp\/v2\/categories?post=86656"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/ekamu.net\/index.php\/wp-json\/wp\/v2\/tags?post=86656"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}