Connection between the cme velocities and decameter radio bursts parameters from URAN-4 observations

dc.contributor.author	Halanin, V. V.
dc.contributor.author	Isaeva, E. A.
dc.contributor.author	Kravetz, R. O.
dc.date.accessioned	2017-05-18T12:04:45Z
dc.date.available	2017-05-18T12:04:45Z
dc.date.issued	2015
dc.description.abstract	The paper reports the results of the research of connection between the coronal mass ejections (CME) with the IV type continual decameter bursts parameters. As the parameters characterizing the CME velocity, we used the integrated flux of the radio bursts and background intensity on 20 and 25 MHz frequencies. The analysis demonstrated that the connection between the CME velocity and IV type bursts increases, if we take into account the intensity of the radio bursts and background on two polarizations at a given frequency. In this case, the correlation coefficient is ≈ 0.75.	uk
dc.identifier.citation	Odessa Astronomical publications = Одесские астрономические публикации = Одеські астрономічні публікації	uk
dc.identifier.uri	https://dspace.onu.edu.ua/handle/123456789/9815
dc.language.iso	en	uk
dc.publisher	Одеський національний університет імені І. І. Мечникова	uk
dc.relation.ispartofseries	;Vol. 28, iss. 2.
dc.subject	coronal mass ejection	uk
dc.subject	radio burst	uk
dc.title	Connection between the cme velocities and decameter radio bursts parameters from URAN-4 observations	uk
dc.type	Article	uk

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