On the recording of regions with increased plasma density on the sun

Details On the recording of regions with increased plasma density on the sun On the recording of regions with increased plasma density on the sun

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992soph..139..275k&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 139, no. 2, June 1992, p. 275-277.

Physics

Balmer Series, H Alpha Line, Plasma Density, Solar Flares, Solar Spectra, Electron Density (Concentration), Optical Filters, Solar Atmosphere, Visible Spectrum

Scientific paper

For the purpose of studying the statistics, dynamics, and morphology of parts of the solar surface with enhanced emission measure and considerable inhomogeneities of electron concentration, it is suggested that a new type of solar observation be introduced: taking filtergrams by means of interference filters, calculated for the Balmer continuum limit and the region of the blue continuum. To determine accurately the inhomogeneity of the electron concentration in an object, it is suggested to scan the surface of the object and record the spectrum of the blue continuum by means of a spectrochronograph.

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