Conference paper or proceedings

Spectra of Solar Magnetic Fields and Diffusion

The Scaling of a time series of magnetic and Doppler images obtained in good seeing conditions at San Fernando Observatory are studied. It is shown that the distribution of scaling exponents (the signularity spectrum) is stable within the time period used (several hours). Two scaling parameters of the space-time power spectrum were found to characterize the turbulent diffusion of solar magnetic fields.

Relationships

Items