1. IIA Institutional Repository
  2. IIAP Publications
  3. IIAP Publications
Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/8026
Full metadata record
DC FieldValueLanguage
dc.contributor.authorRamesh, R-
dc.contributor.authorKathiravan, C-
dc.contributor.authorEbenezer, E-
dc.date.accessioned2022-08-24T05:48:10Z-
dc.date.available2022-08-24T05:48:10Z-
dc.date.issued2022-06-10-
dc.identifier.citationThe Astrophysical Journal, Vol. 932, No. 1, 48en_US
dc.identifier.issn1538-4357-
dc.identifier.urihttp://hdl.handle.net/2248/8026-
dc.descriptionOpen Accessen_US
dc.descriptionOriginal content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.-
dc.description.abstractIt is well known that magnetic field strength (B) in the solar corona can be calculated using the Alfvén Mach number (MA) and Alfvén speed (vA) of the magnetohydrodynamic shock waves associated with coronal type II radio bursts. We show that observations of weak circularly polarized emission associated with the harmonic component of the type II bursts provide independent and consistent estimates of B. For the coronal type II burst observed on 2021 October 9, we obtained B ≈1.5 G and ≈1.9 G at a heliocentric distance (r) of ≈1.8 Re, using the above two techniques, respectively.en_US
dc.language.isoenen_US
dc.publisherAmerican Astronomical Societyen_US
dc.relation.urihttps://doi.org/10.3847/1538-4357/ac6f05-
dc.rights© 2022 The Author(s)-
dc.subjectSolar coronal mass ejectionsen_US
dc.subjectThe Sunen_US
dc.subjectSolar magnetic fieldsen_US
dc.subjectSolar radio emissionen_US
dc.subjectSolar coronaen_US
dc.titleCircular Polarization Observations of Type II Solar Radio Bursts and the Coronal Magnetic Fielden_US
dc.typeArticleen_US
Appears in Collections:IIAP Publications

Files in This Item:
File Description SizeFormat 
Circular Polarization Observations of Type II Solar Radio Bursts and the Coronal Magnetic Field.pdf801.47 kBAdobe PDFView/Open
Show simple item record


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