Oct 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982jbis...35..434s&link_type=abstract
British Interplanetary Society, Journal (Space Chronicle), vol. 35, Oct. 1982, p. 434-440.
Physics
Solar Physics, Sunspots, Solar Constant, Solar Flares, Solar Maximum Mission, Solar X-Rays
Scientific paper
The sun is a stable, mediocre star with a diameter of 1.4 x 10 to the 6th km, mass 2 x 10 to the 30th kg, spectral class early G, and not too far removed on the main sequence of the Hertzsprung-Russell diagram from the category of stars known as red dwarfs. It is said to be stable only when it is compared with other stars in the Galaxy, some of which are clearly very unsteady. However, despite its poor showing in the league table of variability, now that the means of probing the sun through the ingenuity of modern science are available, it is discovered that by terrestrial standards the sun is more violent and turbulent than anything which could be conceived by man.
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