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- W1964444671 abstract "view Abstract Citations (131) References (21) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS The steady global corona Steinolfson, R. S. ; Suess, S. T. ; Wu, S. T. Abstract The formation of the steady coronal structure which consists of coronal streamers and holes is seen in terms of a model employing numerical solutions of time-dependent, dissipationless, magnetohydrodynamic equations of motion applicable to the meridional plane. A coronal streamer consists of closed magnetic field lines near the solar surface with overlying and adjacent open field lines, and the atmosphere, which is stationary in the closed region, flows outward in the open region, or coronal hole. The steady coronal structure is obtained by starting the numerical calculation with a state comprising a polytropic, hydrodynamical solution to the steady-state radial equation of motion coupled with a dipole magnetic field. Global coronal configurations are calculated for values of the plasma beta which vary from 0.1 to 100. It is found that the height and lateral extension of the closed region are only weakly dependent on the data. Publication: The Astrophysical Journal Pub Date: April 1982 DOI: 10.1086/159872 Bibcode: 1982ApJ...255..730S Keywords: Coronal Holes; Magnetohydrodynamic Flow; Plasma Dynamics; Solar Corona; Solar Magnetic Field; Beta Factor; Isothermal Flow; Lines Of Force; Steady State; Stellar Models; Solar Physics full text sources ADS |" @default.
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- W1964444671 date "1982-04-01" @default.
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- W1964444671 title "The steady global corona" @default.
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