Numerical simulations of the K-corona and of the lambda 5303 emission line corona

Details Numerical simulations of the K-corona and of the lambda 5303 emission line corona Numerical simulations of the K-corona and of the lambda 5303 emission line corona

Apr 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981soph...70..229p&link_type=abstract

Solar Physics, vol. 70, Apr. 1981, p. 229-235.

Physics

2

Electron Density Profiles, Solar Corona, Solar Magnetic Field, Solar Simulation, Emission Spectra, Heterogeneity, Hydrostatics, Isophotes

Scientific paper

A numerical simulation of the K-corona and the 4303-A emission line
corona is performed on the basis of the assumption that the corona in
this region is arch-structured. It is shown that material missing in
previous studies is largely confined at the bases of very high arches
and possibly in open structures.

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