Solar structure and evolution

摘要: The Sun provides a critical benchmark for the general study of stellar structure and evolution. Also, knowledge about internal properties is important understanding solar atmospheric phenomena, including magnetic cycle. Here I provide brief overview theory evolution, physical processes parameters that are involved. This followed by discussion extending from birth to latest stages. As background interpretation observations related interior rather extensive analysis sensitivity models assumptions underlying their calculation. then discuss detailed information has become available through helioseismic investigations detection neutrinos, with further constraints provided observed abundances lightest elements. Revisions in determination surface have led increased discrepancies, discussed some detail, between observational inferences models. finally briefly address relation other similar stars prospects asteroseismic