Low-frequency magneto-acoustic waves in the solar chromosphere

Stuart M. Jefferies, Scott W. McIntosh, James D. Armstrong, Thomas J. Bogdan, Alessandro Cacciani, Bernhard Fleck

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

1 Scopus citations

Abstract

We show that inclined magnetic field lines at the boundaries of large-scale convective cells (supergranules) provide "portals" through which low-frequency (< 5 mHz) magneto-acoustic waves can propagate into the solar chromosphere. The energy flux carried by these waves at a height of 400 km above the solar surface, is found to be a factor of four greater than that carried by the high-frequency (> 5 mHz) acoustic waves, which are believed to provide the dominant source of wave heating of the chromosphere. This result opens up the possibility that low-frequency magneto-acoustic waves provide a significant source of energy for balancing the radiative losses of the ambient solar chromosphere.

Original languageEnglish
Title of host publicationSOHO 18/GONG 2006/HELAS I Beyond the spherical Sun
StatePublished - Oct 2006
Externally publishedYes
EventSOHO 18/GONG 2006/HELAS I Beyond the spherical Sun - Sheffield, United Kingdom
Duration: Aug 7 2006Aug 11 2006

Publication series

NameEuropean Space Agency, (Special Publication) ESA SP
Volume624 SP
ISSN (Print)0379-6566

Conference

ConferenceSOHO 18/GONG 2006/HELAS I Beyond the spherical Sun
Country/TerritoryUnited Kingdom
CitySheffield
Period08/7/0608/11/06

Keywords

  • Sun: chromosphere
  • Sun:atmospheric motions
  • Sun:magnetic fields

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