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