Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7768
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dc.contributor.authorRamesh, R-
dc.contributor.authorAnshu Kumari-
dc.contributor.authorKathiravan, C-
dc.contributor.authorKetaki, D-
dc.contributor.authorWang, T. J-
dc.date.accessioned2021-07-02T10:47:03Z-
dc.date.available2021-07-02T10:47:03Z-
dc.date.issued2021-04-28-
dc.identifier.citationGeophysical Research Letters, Vol. 48, No. 8, e2020GL091048en_US
dc.identifier.issn1944-8007-
dc.identifier.urihttp://hdl.handle.net/2248/7768-
dc.descriptionRestricted Accessen_US
dc.description.abstractWe report observations of thermal emission from the frontal structure of a coronal mass ejection (CME) using data obtained with the Gauribidanur RAdioheliograPH simultaneously at 80 and 53 MHz on May 1, 2016. The CME was due to activity on the far side of the Sun, but near its limb. No nonthermal radio burst activity was noticed. This provided an opportunity to observe the faint thermal radio emission from the CME, and hence directly estimate the electron density, mass, and magnetic field strength of the plasma entrained in the CME. Considering that CMEs are mostly observed only in whitelight and reports on their plasma characteristics are also limited, the rare direct radio observations of thermal emission from a CME and independent diagnosis of its plasma parameters are important measurements in the field of CME physics.en_US
dc.language.isoenen_US
dc.publisherAmerican Geophysical Unionen_US
dc.relation.urihttps://doi.org/10.1029/2020GL091048-
dc.rights© American Geophysical Union-
dc.titleNew results on the direct observations of thermal radio emission from a solar coronal mass ejectionen_US
dc.typeArticleen_US
Appears in Collections:IIAP Publications



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