MHD Waves Propogation and Heating of Solar Atmosphere

Details MHD Waves Propogation and Heating of Solar Atmosphere MHD Waves Propogation and Heating of Solar Atmosphere

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agusmsh12a..04b&link_type=abstract

American Geophysical Union, Spring Meeting 2005, abstract #SH12A-04

Physics

7507 Chromosphere

Scientific paper

We examine oscillations in isolated three bright points co-temporal and co-spatial in photosphere and chromosphere in G-band and Ca II K line. Wavelet analysis was used to study wave packets and identify traveling magnetohydrodynamic waves. In general, it is thought likely that the photosphere and chromosphere oscillates in response to forcing by p-modes and granular buffeting, but they are also influenced strongly by presence of magnetic fields. The observed oscillations reveals evidence for kink-mode waves, traveling up through the chromosphere and coupling with sausage-modes waves. This provides a means for energy depositing in the upper chromosphere.

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