Generation of Flows in the Solar Chromosphere Due to Magnetofluid Coupling
نویسندگان
چکیده
It is shown that a generalized magneto–Bernoulli mechanism can effectively generate high velocity flows in the Solar chromosphere by transforming the plasma pressure energy into kinetic energy. It is found that at reasonable heights and for realistic plasma parameters, there is a precipitous pressure fall accompanied by a sharp amplification of the flow speed. Subject headings: Sun: atmosphere — Sun: chromosphere — Sun: corona — Sun: magnetic fields — Sun: transition region Permanent address: Plasma Physics Department, Tbilisi State University, Tbilisi 380028, Georgia Electronic mail: [email protected] Electronic mail: [email protected] Electronic mail: [email protected] [email protected] Electronic mail: [email protected]
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