Study of MHD modes of Oscillations in Solar Coronal arcades
Author & Affiliation:
Seema Pande
Department of Physics, Kumaun Universiry, Nainital (INDIA)
Bimal Pande
Department of Physics, Kumaun Universiry, Nainital (INDIA)
Kavita Pandey
Department of Physics, Kumaun Universiry, Nainital (INDIA)
Keyword:
modes, Oscillations, Solar Coronal
Issue Date:
April 2008
Abstract:
We have made an attempt to study magnetohydrodynamic (MHD) disturbances inside the coronal arcades by solving a pair of second-order two dimensional partial differential equations. MHD modes of oscillations of coronal arcades are investigated. It has been shown that the factors responsible for oscillatory modes give rise to the propagation of MHD waves.
Pages:
27-34
ISSN:
2319-8052 (Online) - 2231-3478 (Print)
Source:
PDF:
DOI:
jusps-B
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Copy the following to cite this article:
S. Pande; B. Pande; K. Pandey, "Study of MHD modes of Oscillations in Solar Coronal arcades", Journal of Ultra Scientist of Physical Sciences, Volume 20, Issue 1, Page Number 27-34, 2018Copy the following to cite this URL:
S. Pande; B. Pande; K. Pandey, "Study of MHD modes of Oscillations in Solar Coronal arcades", Journal of Ultra Scientist of Physical Sciences, Volume 20, Issue 1, Page Number 27-34, 2018Available from: http://www.ultraphysicalsciences.org/paper/1355/
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