Solar evolution

Details Solar evolution Solar evolution

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989gpc.....1...35g&link_type=abstract

Global and Planetary Change (ISSN 0921-8181), vol. 1, Jan. 1989, p. 35-55.

Physics

4

Solar Physics, Stellar Evolution, Stellar Luminosity, Stellar Models, Stellar Structure, Partial Differential Equations, Solar Cycles, Solar Neutrinos, Solar X-Rays, Ultraviolet Radiation

Scientific paper

The standard theory of solar evolution states that luminosity has smoothly risen from an initial level of 70 percent of the current value. Recent ideas suggest a scenario in which the luminosity was never far below current levels, but this remains highly speculative. There is no adequate theory of the solar cycle. Several physical mechanisms have been proposed that could lead to luminosity variations on many time scales.

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