A study of coronal structures in a non-magnetic star

Details A study of coronal structures in a non-magnetic star A study of coronal structures in a non-magnetic star

Oct 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975stin...7610949.&link_type=abstract

Final Report Grambling Coll., LA. Dept. of Physics.

Physics

Magnetic Stars, Perturbation, Solar Corona, Computer Programs, Solar Wind

Scientific paper

Convective instability in the solar corona growth, especially linear growth, was studied. An investigation was also made of nonlinear instability development on a computer. The computer was used to follow a growing perturbation from a small local enhancement in the density of the solar wind to a large increase in the density which would look like one of the rays seen in the sun's corona.

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