Spatial energy spectra of the velocity and magnetic fields in solar active regions

Details Spatial energy spectra of the velocity and magnetic fields in solar active regions Spatial energy spectra of the velocity and magnetic fields in solar active regions

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26a...127..140b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 127, no. 1, Oct. 1983, p. 140-144. Research supported by the Delegation Genera

Physics

1

Energy Spectra, Solar Magnetic Field, Sunspots, Velocity Distribution, Data Reduction, Magnetohydrodynamic Turbulence, Solar Activity, Solar Physics

Scientific paper

Two-dimensional spatial energy spectra for the magnetic and kinetic fields in solar active regions are computed from observations. By averaging over azimuth, one-dimensional spectra are obtained and corrections for atmospheric degradation are performed. The resulting profiles are compared with the observational spectra and the theory published by other authors.

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