Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987azh....64.1088z&link_type=abstract
Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 64, Sept.-Oct. 1987, p. 1088-1093. In Russian.
Astronomy and Astrophysics
Astronomy
Millimeter Waves, Radio Frequencies, Solar Activity, Solar Radio Emission, Spectrum Analysis, Stellar Models, Centimeter Waves, Chromosphere, Plasma Density, Solar Corona, Solar Temperature
Scientific paper
The features of the frequency spectrum of the s-component of solar radio emission in the millimeter and short-wave part of the centimeter range are considered. The physical conditions in the generation region (temperature, and chromospheric and coronal densities) which determine the form of different frequency spectra are studied. This may be a monotonic decrease in intensity with wavelength or a complex spectrum with a minimum intensity at a wavelength of less than about 2 cm and increasing intensity toward shorter wavelengths.
No associations
LandOfFree
The interpretation of the frequency spectrum of millimeter-wave radiation from solar active regions does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The interpretation of the frequency spectrum of millimeter-wave radiation from solar active regions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The interpretation of the frequency spectrum of millimeter-wave radiation from solar active regions will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1774016