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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5929

Title: Nature of quiet Sun oscillations using data from the hinode, TRACE, and SOHO spacecraft
Authors: Gupta, G. R
Subramanian, S
Banerjee, D
Madjarska, M. S
Doyle, J. G
Keywords: Chromosphere, quiet
Transition region
Oscillations
MHD waves
Issue Date: Jan-2013
Publisher: Springer
Citation: Solar physics, Vol. 282, No. 1, pp. 67-86
Abstract: We study the nature of quiet-Sun oscillations using multi - wavelength observations from TRACE, Hinode, and SOHO. The aim is to investigate the existence of propagating waves in the solar chromosphere and the transition region by analyzing the statistical distribution of power in different locations, e.g. in bright magnetic (network), bright non-magnetic and dark non-magnetic (inter-network) regions, separately. We use Fourier power and phase-difference techniques combined with a wavelet analysis. Two-dimensional Fourier power maps were constructed in the period bands 2 – 4 minutes, 4 – 6 minutes, 6 – 15 minutes, and beyond 15 minutes. We detect the presence of long-period oscillations with periods between 15 and 30 minutes in bright magnetic regions. These oscillations were detected from the chromosphere to the transition region. The Fourier power maps show that short-period powers are mainly concentrated in dark regions whereas long-period powers are concentrated in bright magnetic regions. This is the first report of long-period waves in quiet-Sun network regions. We suggest that the observed propagating oscillations are due to magneto acoustic waves, which can be important for the heating of the solar atmosphere.
Description: Restricted Access
The original publication is available at springerlink.com
URI: http://hdl.handle.net/2248/5929
ISSN: 1573-093X
Alternative Location: http://dx.doi.org/10.1007/s11207-012-0146-y
http://arxiv.org/abs/1209.5252
Copyright: © Springer
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