INational Science Foundation (NSF) yethule izithombe ezinemininingwane eminingi yobuso beLanga ezithathwe kuze kube manje.
Ukudubula kwenziwe kusetshenziswa i-Daniel K. Inouye Solar Telescope (DKIST). Le divayisi, etholakala e-Hawaii, ifakwe isibuko esingamamitha angu-4. Kuze kube manje, i-DKIST isibonakude esikhulu kunazo zonke esiklanyelwe ukufunda inkanyezi yethu.
Idivayisi iyakwazi "ukuhlola" ukwakheka ebusweni beLanga kusuka ngobukhulu obusuka ku-30 ββkm ububanzi. Isithombe esiveziwe sibonisa ngokusobala ukwakheka kwamaselula: ubukhulu bendawo ngayinye buqhathaniswa nendawo yesifunda saseMelika saseTexas.
Izindawo ezikhanyayo kumaseli yizoni lapho i-plasma ibalekela khona ebusweni beLanga, futhi imiphetho emnyama yilapho ishona khona emuva. Le nqubo ibizwa ngokuthi i-convection.
Kulindeleke ukuthi i-Daniel Inouye Solar Telescope izosivumela ukuthi siqoqe idatha emisha mayelana nenkanyezi yethu futhi sicwaninge ngokuxhumanisa kwelanga nomhlaba, noma lokho okubizwa ngokuthi isimo sezulu sasemkhathini, ngemininingwane eyengeziwe. Njengoba kwaziwa, umsebenzi eLangeni uthinta i-magnetosphere, ionosphere nomkhathi woMhlaba.
Source: 3dnews.ru