Routine Characterization of Coronal Mass Ejections Using Gyrosynchrotron Emission

  • Divya Oberoi
  • , Devojyoti Kansabanik
  • , Surajit Mondal

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

Abstract

Coronal magnetic fields are understood to be the drivers of space weather, though their measurements have remained challenging. Due to the nature of the emission mechanisms involved, the polarization properties of coronal radio emissions are sensitive to coronal magnetic fields. Here we summarize the recent progress in measuring and modeling the gyrosynchrotron emissions from coronal mass ejections (CMEs) at meter wavelengths and justify our expectations for this method to become a routine tool for estimating the magnetic fields trapped in CMEs and other physical parameters of CME plasma.

Original languageEnglish
Title of host publication2023 35th General Assembly and Scientific Symposium of the International Union of Radio Science, URSI GASS 2023
PublisherInstitute of Electrical and Electronics Engineers Inc.
ISBN (Electronic)9789463968096
DOIs
StatePublished - 2023
Event35th General Assembly and Scientific Symposium of the International Union of Radio Science, URSI GASS 2023 - Sapporo, Japan
Duration: Aug 19 2023Aug 26 2023

Publication series

Name2023 35th General Assembly and Scientific Symposium of the International Union of Radio Science, URSI GASS 2023

Conference

Conference35th General Assembly and Scientific Symposium of the International Union of Radio Science, URSI GASS 2023
Country/TerritoryJapan
CitySapporo
Period08/19/2308/26/23

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