A cikin 1612, Galileo Galili Galile ya yi nazarin rana tare da telescope, aiwatar da hoton a kan farin allon. A cikin haske mai haske, duhu mai haskakawa kuma ya fasa kananan duhu duhu. Yayi nesa da farkon gano ruwan rana - game da kasancewar su da aka sani da zurfin tsufa. Koyaya, Galili Galili ya kusanta su da babban daidaito, kuma har yanzu ana kiyaye waɗannan hotunan.
A yau, rana tana cikin binciken mafi ban mamaki da kuma m na'urori na'urori. Sun "gani" tauraron a cikin waƙoƙi daban-daban na rajista magnetic filayen da ayyukansa ke haifar da bayyanar da aibobi, da kuma samarwa, da kuma wasu abubuwan da suka yi a rana. Koyaya, zane Galili yana da darajar rarrabuwa - tarihi: an yi halitta an lokacin da babu wasu kayan aikin, kuma kawai suka riƙe bayanan akan ayyukan rana shekaru 400 da suka gabata.
Kwanan nan, ƙungiyar masu haɓakawa daga Jami'ar Konchi a cikin Seobel sun kirkiro hanyar sadarwa ta Heliophys - da Ba'amurke Binciken Ba'amurke ya yi aiki a UV Band. Sakamakon wannan aikin an gabatar da shi a cikin labarin da aka buga a cikin Journal Mobilysical.
Don horar da samfurin, masana kimiyya sun juya ga tarin bayanan da ke lura Wilson, inda tun daga 1912 kuma - har yanzu suna yin zane-zanen rana da kuma aibobi. Bayan cika hotuna na 2011-015, an tabbatar dasu ta hotunan UV da bayanan SDE Magnetometer, wanda aka yi a ranakun da ya dace. Wannan jerin abubuwa ana amfani da su don koyar da cibiyar sadarwa ta.
A ƙarshe, an gabatar da zane Galili a cikin tsarin - kuma ya sami damar sake gina kwatancen hotunan SDDeic, wanda a cikin 1812, a cikin kusanci da dogon lokaci aibobi. Masana kimiyya suna fatan inganta cibiyar sadarwar su da amfani da shi don sake gina rana, jan hankali da sauran masana taurari na baya.
Source: Kimiyya mara kyau