{"id":22594,"date":"2025-02-18T09:17:02","date_gmt":"2025-02-18T09:17:02","guid":{"rendered":"https:\/\/www.starhuntereos.com\/heliophysics\/?page_id=22594"},"modified":"2025-02-22T00:34:29","modified_gmt":"2025-02-22T00:34:29","slug":"tompok-matahari","status":"publish","type":"page","link":"https:\/\/www.starhuntereos.com\/heliophysics\/tompok-matahari\/","title":{"rendered":"Tompok Matahari"},"content":{"rendered":"

[vc_row row_type=”row” use_row_as_full_screen_section=”no” type=”full_width” text_align=”left” background_animation=”none” padding_bottom=”45″ css_animation=””][vc_column width=”1\/2″]

Tompok Matahari (Sun spot)<\/span><\/div>[vc_separator type=”transparent” border_style=”” up=”20″ down=”0″ icon_pack=”font_awesome”][vc_column_text]Sunspot adalah kawasan yang lebih sejuk di permukaan Matahari yang disebabkan oleh penumpuan garis medan magnet. [\/vc_column_text][vc_separator type=”transparent” border_style=”” up=”20″ down=”0″ icon_pack=”font_awesome”][vc_column_text]Berikut adalah ringkasan daripada penerangan anda:[\/vc_column_text][vc_separator type=”transparent” border_style=”” up=”20″ down=”0″ icon_pack=”font_awesome”][vc_column_text]Medan Magnet dan Plasma<\/strong>: Sunspot terbentuk akibat garis medan magnet yang berpusing dan terganggu yang disebabkan oleh plasma Matahari, iaitu gas yang bercas elektrik. Gangguan magnetik ini menghalang haba daripada sampai ke permukaan Matahari, menjadikan sunspot lebih sejuk dan gelap berbanding kawasan sekitarnya.[\/vc_column_text][\/vc_column][vc_column width=”1\/2″][vc_single_image image=”22865″ img_size=”full” qode_css_animation=””][vc_separator type=”transparent” border_style=”” up=”20″ down=”0″ icon_pack=”font_awesome”][vc_column_text]<\/p>\n
Imej kumpulan sunspot yang besar dari NASA\u2019s Solar Dynamics Observatory adalah rujukan visual yang sangat baik untuk fenomena ini.<\/h6>\n

[\/vc_column_text][\/vc_column][\/vc_row][vc_row row_type=”row” use_row_as_full_screen_section=”no” type=”full_width” text_align=”left” background_animation=”none” padding_bottom=”45″ css_animation=””][vc_column][vc_column_text]<\/p>\n

Kumpulan Sunspot dan Kawasan Aktif<\/strong>: Sunspot sering ditemui di “kawasan aktif” Matahari, di mana medan magnet yang kuat berinteraksi dengan atmosfera suria. Kawasan ini terkenal dengan fenomena suria seperti letusan suria dan pelepasan jisim korona, yang boleh memberi kesan kepada Bumi.<\/p>\n

[\/vc_column_text][vc_separator type=”transparent” border_style=”” up=”20″ down=”0″ icon_pack=”font_awesome”][vc_column_text]Mengesan Aktiviti Suria<\/strong>: Jumlah sunspot berbeza sepanjang kitaran suria yang berlangsung selama 11 tahun. Kitaran ini melibatkan tempoh solar minimum (sedikit sunspot) dan solar maksimum (banyak sunspot). NASA dan NOAA mengesan sunspot untuk meramalkan aktiviti suria, seperti ribut suria yang boleh memberi kesan kepada kapal angkasa dan komunikasi.[\/vc_column_text][vc_separator type=”transparent” border_style=”” up=”20″ down=”0″ icon_pack=”font_awesome”][vc_column_text]<\/p>\n

Pada tahun 2019, kitaran suria ke-25 bermula, membantu para saintis memahami dan meramalkan kelakuan Matahari dengan lebih berkesan.<\/p>\n

[\/vc_column_text][vc_separator type=”transparent” border_style=”” up=”20″ down=”0″ icon_pack=”font_awesome”][vc_separator type=”transparent” border_style=”” up=”20″ down=”0″ icon_pack=”font_awesome”][\/vc_column][\/vc_row]<\/p>\n<\/section>","protected":false},"excerpt":{"rendered":"

[vc_row row_type=”row” use_row_as_full_screen_section=”no” type=”full_width” text_align=”left” background_animation=”none” padding_bottom=”45″ css_animation=””][vc_column width=”1\/2″][vc_separator type=”transparent” border_style=”” up=”20″ down=”0″ icon_pack=”font_awesome”][vc_column_text]Sunspot adalah kawasan yang lebih sejuk di permukaan Matahari yang disebabkan oleh penumpuan garis medan magnet. [\/vc_column_text][vc_separator type=”transparent” border_style=”” up=”20″ down=”0″ icon_pack=”font_awesome”][vc_column_text]Berikut adalah ringkasan daripada penerangan anda:[\/vc_column_text][vc_separator type=”transparent” border_style=”” up=”20″ down=”0″ icon_pack=”font_awesome”][vc_column_text]Medan Magnet dan Plasma: Sunspot terbentuk akibat garis medan magnet yang berpusing dan terganggu…<\/p>\n","protected":false},"author":1,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-22594","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/www.starhuntereos.com\/heliophysics\/wp-json\/wp\/v2\/pages\/22594","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.starhuntereos.com\/heliophysics\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/www.starhuntereos.com\/heliophysics\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/www.starhuntereos.com\/heliophysics\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/www.starhuntereos.com\/heliophysics\/wp-json\/wp\/v2\/comments?post=22594"}],"version-history":[{"count":7,"href":"https:\/\/www.starhuntereos.com\/heliophysics\/wp-json\/wp\/v2\/pages\/22594\/revisions"}],"predecessor-version":[{"id":22868,"href":"https:\/\/www.starhuntereos.com\/heliophysics\/wp-json\/wp\/v2\/pages\/22594\/revisions\/22868"}],"wp:attachment":[{"href":"https:\/\/www.starhuntereos.com\/heliophysics\/wp-json\/wp\/v2\/media?parent=22594"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}