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- W52784711 abstract "The Sun is an unspectacular star of spectral type G2 somewhere in the outskirtsof our Milky Way galaxy, where there are millions or even billions of others. Yetit is the only star that can be studied in full detail, and it is the dominant body ofour Solar System and the heliosphere in which it is embedded. The Sun concen-trates almost all of the mass (nearly 99.9%), and it is the only relevant source oflight and energy in the Solar System. Its magnetic field and tenuous outermostatmosphere, the corona and solar wind, permeate all of interplanetary space outto a distance of about 100 astronomical units, far beyond the orbits of the plan-ets. It is therefore worth exploring this medium, not only because astronautsmight want to travel there, but also because it affects all bodies in space, man-made or natural, most notably the Earth itself. This influence would be a rela-tively simple matter were it not for the fact that all solar output, be it radiationor particles, is variable on all time scales from less than minutes to billions ofyears.Several ISSI workshops have addressed themes in this context" @default.
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- W52784711 date "2005-01-01" @default.
- W52784711 modified "2023-09-27" @default.
- W52784711 title "The Sun, from Core to Corona and Solar Wind" @default.
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