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Nonlinear MHD Processes in the Sun’s Atmosphere

1999
The outer atmosphere of the Sun, the corona, is an ionised high temperature plasma that is dominated by the coronal magnetic field. There are many important coronal phenomena that may be modelled as a magnetised fluid and described by the MHD equations.
openaire   +1 more source

The atmosphere of the sun

Vistas in Astronomy, 1988
openaire   +1 more source

Nucleation and Growth of Nanoparticles in the Atmosphere

Chemical Reviews, 2012
Renyi Zhang, Alexei F Khalizov, Lin Wang
exaly  

The Circulation of the Sun's Atmosphere

Scientific American, 1968
Victor P. Starr, Peter A. Gilman
openaire   +1 more source

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