INational Science Foundation (NSF) iveze ezona foto zineenkcukacha zomphezulu weLanga ezithathiweyo ukuza kuthi ga ngoku.
Ukudubula kwenziwa kusetyenziswa iDaniel K. Inouye Solar Telescope (DKIST). Esi sixhobo, esiseHawaii, sixhotyiswe ngesibuko seemitha ezi-4. Ukuza kuthi ga ngoku, i-DKIST yeyona telescope inkulu eyenzelwe ukufunda inkwenkwezi yethu.
Isixhobo siyakwazi "ukuvavanya" iifom ebusweni beLanga ukusuka kwi-30 km ububanzi. Umfanekiso obonisiweyo ubonisa ngokucacileyo ubume beselula: ubungakanani bommandla ngamnye buthelekiswa nommandla welizwe laseMelika laseTexas.
Iindawo eziqaqambileyo kwiiseli ziindawo apho iplasma ibalekela kumphezulu weLanga, kwaye imida emnyama kulapho ibuyela khona. Le nkqubo ibizwa ngokuba yi-convection.
Kulindeleke ukuba iDaniel Inouye Solar Telescope iya kusivumela ukuba siqokelele idatha entsha esemgangathweni malunga neenkwenkwezi zethu kwaye sifunde unxibelelwano lwelanga nomhlaba, okanye okubizwa ngokuba yimozulu yendawo, ngokweenkcukacha ngakumbi. Njengoko kwaziwa, umsebenzi weLanga uchaphazela i-magnetosphere, i-ionosphere kunye nomoya womhlaba.
umthombo: 3dnews.ru