Microscopic spectral features in solar decametric bursts and coronal irregularities.
Abstract
A crossed Yagi antenna array at 35 MHz was employed in conjunction with a polarization switch so as to enable spectral observations of solar noise storm activity in R and L polarizations. Intense decametric solar noise storms were recorded during the third week of November 1975 and fourth week of March 1976 with the help of a high resolution spectroscope operating near 35 MHz.
- Publication:
-
Solar Physics
- Pub Date:
- November 1976
- DOI:
- 10.1007/BF00155309
- Bibcode:
- 1976SoPh...50..481S
- Keywords:
-
- Decametric Waves;
- Radio Spectra;
- Solar Corona;
- Solar Radio Bursts;
- Drift Rate;
- Electron Density (Concentration);
- Electrostatic Waves;
- Linear Arrays;
- Solar Spectra;
- Wave Scattering;
- Yagi Antennas;
- Solar Physics;
- Additional Propagation;
- Propagation Delay;
- Plasma Wave;
- Dynamic Spectrum;
- Langmuir Wave