Detection of MHD waves in the solar chromosphere

Details Detection of MHD waves in the solar chromosphere Detection of MHD waves in the solar chromosphere

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..895...80k&link_type=abstract

FIFTY YEARS OF ROMANIAN ASTROPHYSICS. AIP Conference Proceedings, Volume 895, pp. 80-84 (2007).

Astronomy and Astrophysics

Astrophysics

Chromosphere, Magnetohydrodynamics And Plasmas

Scientific paper

One of the main features of the quiet solar chromosphere is the Network Bright Points (NBP), formed by emerging magnetic flux at the boundaries of supergranular cells. Using SSW IDL routines and wavelet analysis of series of images in four bandpasses (CaIIK3, Mgb1, Mgb2 and Hα core) we have detected MHD wave modes in the Network Bright Points of the solar chromosphere. The observations have been analyzed using cross-correlation techniques and we have drawn conclusions on wave propagation and mode-coupling.

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