Observations and analysis of emission from solar active regions at the edge of the Balmer continuum

Details Observations and analysis of emission from solar active regions at the edge of the Balmer continuum Observations and analysis of emission from solar active regions at the edge of the Balmer continuum

Jun 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997azh....74..460k&link_type=abstract

Astronomicheskij Zhurnal, vol. 74, p. 460

Astronomy and Astrophysics

Astronomy

Solar Activity, Balmer Series, Continuous Spectra, H Alpha Line, Cosmic Plasma, Satellite Observation, Calcium, Electron Density Profiles, Hydrogen Plasma

Scientific paper

The first results of CCD observations of the sun in the Balmer and Paschen continua and in the Balmer precontinuum are presented. The intensity distribution in the Balmer precontinuum in a knot in the active region NOAA/USAF 7890 provides information about inhomogeneities in the electron density of the plasma along the line of sight. The value of conducting monitoring observations of this kind is demonstrated.

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