TY - GEN
T1 - Resonant coupling of solar global oscillations to the solar atmosphere
AU - Pintér, B.
N1 - Copyright:
Copyright 2008 Elsevier B.V., All rights reserved.
PY - 2005
Y1 - 2005
N2 - Traditionally solar global oscillations are considered less important for the dynamics of the solar atmosphere. This thinking has considerably changed in light of the currently available high spatial and time resolution observations, allowing us to perform magnetic atmospheric seismology. In our work we demonstrate how the solar global oscillations interact with the lower parts of the solar atmosphere (chromosphere and transition region). These global oscillations are coupled resonantly to local MHD slow and/or Alfvén waves arising in the inhomogeneous part of the solar atmosphere. Special attention is paid to the efficiency of this resonant interaction in the presence of atmospheric magnetic fields.
AB - Traditionally solar global oscillations are considered less important for the dynamics of the solar atmosphere. This thinking has considerably changed in light of the currently available high spatial and time resolution observations, allowing us to perform magnetic atmospheric seismology. In our work we demonstrate how the solar global oscillations interact with the lower parts of the solar atmosphere (chromosphere and transition region). These global oscillations are coupled resonantly to local MHD slow and/or Alfvén waves arising in the inhomogeneous part of the solar atmosphere. Special attention is paid to the efficiency of this resonant interaction in the presence of atmospheric magnetic fields.
KW - Sun: atmosphere
KW - Sun: helioseismology
KW - Sun: magnetic fields
KW - Sun: oscillations
UR - http://www.scopus.com/inward/record.url?scp=33644788666&partnerID=8YFLogxK
M3 - Conference Proceeding (Non-Journal item)
AN - SCOPUS:33644788666
T3 - European Space Agency, (Special Publication) ESA SP
SP - 461
EP - 464
BT - 11th European Solar Physics Meeting - The Dynamic Sun:
T2 - 11th European Solar Physics Meeting - The Dynamic Sun: Challenges for Theory and Observations
Y2 - 11 September 2005 through 16 November 2005
ER -