Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7203
Title: Strength of the Solar Coronal Magnetic Field – A Comparison of Independent Estimates Using Contemporaneous Radio and White-Light Observations
Authors: Anshu Kumari
Ramesh, R
Kathiravan, C
Wang, T. J
Keywords: Sun;Coronal mass ejections;Radio bursts;Coronal magnetic field
Issue Date: Nov-2017
Publisher: Springer
Citation: Solar Physics, Vol. 292, No. 11, 161
Abstract: We estimated the coronal magnetic field strength (B) during the 23 July 2016 coronal mass ejection (CME) event using i) the flux rope structure of the CME in the white-light coronagraph images and ii) the band-splitting in the associated type II burst. No models were assumed for the coronal electron density (N(r)) we used in the estimation. The results obtained with these two independent methods correspond to different heliocentric distances (r) in the range ≈2.5--4.5 R⊙, but they show excellent consistency and could be fit with a single power-law distribution of the type B(r)=5.7r−2.6 G, which is applicable in that distance range. The power-law index (i.e. −2.6) is in good agreement with the results obtained in previous studies by different methods.
Description: Restricted Access
The original publication is available at springerlink.com
URI: http://hdl.handle.net/2248/7203
ISSN: 0250-6335
???metadata.dc.rights???: © Springer
???metadata.dc.relation.uri???: https://doi.org/10.1007/s11207-017-1180-6
Appears in Collections:IIAP Publications

Files in This Item:
File Description SizeFormat 
Strength of_the_Solar_Coronal.pdfRestricted Access 1.15 MBAdobe PDFView/Open


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.