Integral properties of the magnetic fields of solar active regions under quiet and flare activity conditions

Details Integral properties of the magnetic fields of solar active regions under quiet and flare activity conditions Integral properties of the magnetic fields of solar active regions under quiet and flare activity conditions

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004a%26at...23..525c&link_type=abstract

Astronomical and Astrophysical Transactions, vol. 23, Issue 6, p.525-531

Astronomy and Astrophysics

Astrophysics

6

Scientific paper

The well-known problem of the correlations between eruptive processes in the chromosphere and corona and peculiarities of the magnetic field structure in solar active regions (ARs) on the photospheric level are discussed in this paper. We study the time variations in the first four moments of distribution (over the field) of four integral parameters of the magnetic field of an AR. We used Huairou (PR China) and Solar Orbit Heliospheric Observatory, Michelson-Doppler Interferometer (SOHO/MDI) measurements of longitudinal magnetic fields for ten ARs. We study the following integral parameters of an AR: total magnetic flux Fa, tilting angle An, complexity parameter Hu and relative total magnetic flux imbalance Ov. The distributions of these parameters show essential differences between quiet and flare productive ARs. One can observe specific differences in the distributions before and during flares. The four first distribution moments take into account these differences and so they can be good quantitative parameters of the current states of ARs relative to their flare productivity.

Affiliated with

Also associated with

No associations

Rating

Integral properties of the magnetic fields of solar active regions under quiet and flare activity conditions does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Integral properties of the magnetic fields of solar active regions under quiet and flare activity conditions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Integral properties of the magnetic fields of solar active regions under quiet and flare activity conditions will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-889701