DocumentCode :
3403735
Title :
Spectrum and duration of bursts of solar noise storms
Author :
Yurovsky, Y.F. ; Yurovsky, Y.Y.
Author_Institution :
Crimean Astrophys. Obs., Nauchny
fYear :
2008
fDate :
8-12 Sept. 2008
Firstpage :
872
Lastpage :
873
Abstract :
The method of analysis of random time function is developed by using its timing and spectral description. It was found out that the square-law distribution of bursts duration of noise storms and their hyperbolic spectrum is possible caused by random refraction of radio waves on the inhomogeneities of solar corona.
Keywords :
electromagnetic wave refraction; radiative transfer; random processes; solar corona; solar radiofrequency radiation; solar spectra; time series; hyperbolic spectrum; radiowave random refraction; random time function analysis; solar corona inhomogeneities; solar noise storm duration; solar noise storm spectrum; square law distribution; Helium; Hidden Markov models; IEEE catalog; Indium tin oxide; Microwave technology; Organizing; Storms;
fLanguage :
English
Publisher :
ieee
Conference_Titel :
Microwave & Telecommunication Technology, 2008. CriMiCo 2008. 2008 18th International Crimean Conference
Conference_Location :
Sevastopol, Crimea
Print_ISBN :
978-966-335-166-7
Electronic_ISBN :
978-966-335-169-8
Type :
conf
DOI :
10.1109/CRMICO.2008.4676639
Filename :
4676639
Link To Document :
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