Correlation of hard X-ray and type 3 bursts in solar flares
Technical Report
·
OSTI ID:6168455
Correlations between X-ray and type 3 radio emission of solar bursts are described through a bivariate distribution function. Procedures for determining the form of this distribution are described. A model is constructed to explain the correlation between the X-ray spectral index and the ratio of X-ray to radio intensities. Implications of the model are discussed.
- Research Organization:
- Stanford Univ., CA (USA)
- OSTI ID:
- 6168455
- Report Number(s):
- N-8232243; NASA-CR-169167
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
640104* -- Astrophysics & Cosmology-- Solar Phenomena
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
CORRELATIONS
DISTRIBUTION FUNCTIONS
ELECTROMAGNETIC RADIATION
FUNCTIONS
HARD X RADIATION
IONIZING RADIATIONS
RADIATIONS
SOLAR ACTIVITY
SOLAR FLARES
SOLAR X-RAY BURSTS
SPECTRA
X RADIATION
X-RAY SPECTRA
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
CORRELATIONS
DISTRIBUTION FUNCTIONS
ELECTROMAGNETIC RADIATION
FUNCTIONS
HARD X RADIATION
IONIZING RADIATIONS
RADIATIONS
SOLAR ACTIVITY
SOLAR FLARES
SOLAR X-RAY BURSTS
SPECTRA
X RADIATION
X-RAY SPECTRA