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Volume : III, Issue : I, February - 2013 MAGNETISM OF THE SUN CHANDRAKANT L. TUMBADE DOI : 10.9780/22307850, Published By : Laxmi Book Publication Abstract : The Sun is a magnetically active star. It supports a strong, changing magnetic
field that varies year-to-year and reverses direction about every eleven years around
solar maximum. The Sun's magnetic field leads to many effects that are collectively
called solar activity, including sunspots on the surface of the Sun, solar flares, and
variations in solar wind that carry material through the Solar System. For study of
magnetism of the Sun i.e. Solar Magnetism. Magnetic fields are present almost
everywhere on the Sun. Without these fields the Sun would have been a rather dull object. Keywords : Article : Cite This Article : CHANDRAKANT L. TUMBADE, (2013). MAGNETISM OF THE SUN. Indian Streams Research Journal, Vol. III, Issue. I, DOI : 10.9780/22307850, http://oldisrj.lbp.world/UploadedData/1956.pdf References : - Zeeman, P. (1897). 'On the influence of Magnetism on the Nature of the Light emitted by a Substance'.Phil. Mag. 43:226.
- Babcock, H. W. & Babcock, H. D. 1958, Photospheric magnetic fields, Vol. 6, Electromagnetic Phenomena in Cosmical Physics, ed. B. Lehnert, 239
- G.E. Hale, On the probable existence of a magnetic fields in sunspots. Astrophys. J. 28, 315343
- Woolfson,M (2000). "The origin and evolution of the solar system". 41-47
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