|Author||Waldron, W. L. ♦ Mullan, D. J.|
|Source||United States Department of Energy Office of Scientific and Technical Information|
|Subject Keyword||CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS ♦ SOLAR CORONA ♦ MAGNETOHYDRODYNAMICS ♦ CHEMICAL COMPOSITION ♦ MAGNETIC FIELDS ♦ MASS TRANSFER ♦ NUMERICAL ANALYSIS ♦ PHOTOSPHERE ♦ SOLAR WIND ♦ STAR MODELS ♦ TWO-DIMENSIONAL CALCULATIONS ♦ ATMOSPHERES ♦ FLUID MECHANICS ♦ HYDRODYNAMICS ♦ MATHEMATICAL MODELS ♦ MATHEMATICS ♦ MECHANICS ♦ SOLAR ACTIVITY ♦ SOLAR ATMOSPHERE ♦ STELLAR ATMOSPHERES ♦ STELLAR CORONAE ♦ Astrophysics & Cosmology- Solar Phenomena|
|Abstract||Coronal bright points are known to be magnetic in nature. A two-dimensional MHD code was devleoped to investigate the rsponse of a stratified atmosphere to a localized magnetic structure. If a bright point occurs at a region where flux tubes of opposite polarity have encountered by chance it is found that, in the presence of stratification, a net upward mass flux results. Upflow velocities of up to one half of the Alfven speed are produced. The implications of the results for mass outflows from bright points in coronal holes are discussed. 24 references.|
|Learning Resource Type||Article|
|Publisher Department||Applied Research Corp., Landover, MD ♦ Franklin Institute, Newark, DE|
|Publisher Place||United States|
|Organization||Applied Research Corp., Landover, MD ♦ Franklin Institute, Newark, DE|
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