The photospheric magnetic field response to a solar flare.

Details The photospheric magnetic field response to a solar flare. The photospheric magnetic field response to a solar flare.

Jun 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998kfnt...14..210a&link_type=abstract

Kinematika Fiz. Nebesn. Tel, Tom 14, No. 3, p. 210 - 218

Physics

1

Solar Magnetic Fields: Solar Flares, Solar Magnetic Fields: Solar Photosphere

Scientific paper

Using the vector magnetic field measurements the authors have studied the scaling of photospheric magnetic field and current helicity Bz·(∇×B)z during the periods of high flare activity in two active regions. The results allow to assume that from the very onset of a flare the transverse photospheric magnetic field undergoes significant changes, namely, the fluctuations energy is reduced as well as the spatial structure gets more simple: the transverse field becomes more smooth what seems to be explained by the dissipation of the pre-existing internal tangential discontinuities.

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