{"id":22860,"date":"2011-11-29T11:37:15","date_gmt":"2011-11-29T08:37:15","guid":{"rendered":"http:\/\/www.fyysika.ee\/uudised\/?p=22860"},"modified":"2011-11-29T11:37:15","modified_gmt":"2011-11-29T08:37:15","slug":"vaike-leek-valgustab-supernoovade-plahvatusi","status":"publish","type":"post","link":"https:\/\/www.fyysika.ee\/?p=22860","title":{"rendered":"V\u00e4ike leek valgustab supernoovade plahvatusi"},"content":{"rendered":"<div id=\"attachment_22859\" style=\"width: 570px\" class=\"wp-caption aligncenter\"><a href=\"http:\/\/www.fyysika.ee\/uudised\/wp-content\/uploads\/2011\/11\/111122113214-large.jpg\"><img loading=\"lazy\" decoding=\"async\" aria-describedby=\"caption-attachment-22859\" class=\"size-full wp-image-22859 \" src=\"http:\/\/www.fyysika.ee\/uudised\/wp-content\/uploads\/2011\/11\/111122113214-large.jpg\" alt=\"\" width=\"560\" height=\"280\" srcset=\"https:\/\/www.fyysika.ee\/wp-content\/uploads\/2011\/11\/111122113214-large.jpg 800w, https:\/\/www.fyysika.ee\/wp-content\/uploads\/2011\/11\/111122113214-large-300x150.jpg 300w, https:\/\/www.fyysika.ee\/wp-content\/uploads\/2011\/11\/111122113214-large-250x125.jpg 250w\" sizes=\"auto, (max-width: 560px) 100vw, 560px\" \/><\/a><p id=\"caption-attachment-22859\" class=\"wp-caption-text\">Kujutis neljast erinevatel aegadel v\u00f5etud kaadrist, mis n\u00e4itab tule levimist esialgselt alahelikiirusel suunaga v\u00e4ljapoole. Saavutades teatud tiheduse (m\u00e4rgitud rohelisega), muutub leek plahvatuseks. Reaktsiooni kulu muutuja on m\u00e4rgitud v\u00e4rviliselt, n\u00e4idates tuuma statistilise pool-tasakaalu (nuclear statistical quasi-equilibrium) produktide p\u00f5lemist tuuma statistilise tasakaalu produktideks. Sinine kontuur m\u00e4rgib eraldust eelnevalt soojust juhtiva tuuma ja isotermilise v\u00e4liskihi vahel. Parempoolse kujutise skaala on teistest kujutistest suurem. Pilt: Aaron Jackson<\/p><\/div>\n<p>Alustades v\u00e4ikeste leekide k\u00e4itumise uurimist laboris, on uurijate meeskond saanud uusi teadmisi j\u00f5udude kohta, mis juhivad 1a t\u00fc\u00fcpi supernoovade plahvatusi. Need t\u00e4heplahvatused on Universumi evolutsiooni uurimise\u00a0olulisteks vahenditeks ja seega v\u00f5ib parem arusaam nende k\u00e4itumisest aidata vastata m\u00f5nele astronoomia p\u00f5hik\u00fcsimusele.<\/p>\n<p><a href=\"http:\/\/www.sciencedaily.com\/releases\/2011\/11\/111122113214.htm\">Allikas<\/a><\/p>\n<p>Teadusartikkel: ,,<a href=\"http:\/\/meetings.aps.org\/Meeting\/DFD11\/Event\/155293\">Turbulence and Combustion in Type Ia Supernovae<\/a>&#8220;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Alustades v\u00e4ikeste leekide k\u00e4itumise uurimist laboris, on uurijate meeskond saanud uusi teadmisi j\u00f5udude kohta, mis juhivad 1a t\u00fc\u00fcpi supernoovade plahvatusi. Need t\u00e4heplahvatused on Universumi evolutsiooni uurimise\u00a0olulisteks vahenditeks ja seega v\u00f5ib parem arusaam nende k\u00e4itumisest aidata vastata m\u00f5nele astronoomia p\u00f5hik\u00fcsimusele. Allikas Teadusartikkel: ,,Turbulence and Combustion in Type Ia Supernovae&#8220;<\/p>\n","protected":false},"author":448,"featured_media":22859,"comment_status":"open","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"_genesis_hide_title":false,"_genesis_hide_breadcrumbs":false,"_genesis_hide_singular_image":false,"_genesis_hide_footer_widgets":false,"_genesis_custom_body_class":"","_genesis_custom_post_class":"","_genesis_layout":"","footnotes":""},"categories":[40],"tags":[],"class_list":{"0":"post-22860","1":"post","2":"type-post","3":"status-publish","4":"format-standard","5":"has-post-thumbnail","7":"category-paev-pildis","8":"entry"},"_links":{"self":[{"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=\/wp\/v2\/posts\/22860","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=\/wp\/v2\/users\/448"}],"replies":[{"embeddable":true,"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=22860"}],"version-history":[{"count":0,"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=\/wp\/v2\/posts\/22860\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=\/wp\/v2\/media\/22859"}],"wp:attachment":[{"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=22860"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=22860"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.fyysika.ee\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=22860"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}