Have a look at: Atlas of magnetic fields
- compiled from data observed with the Effelsberg, VLA and ATCA radio telescopes
Home Page of Marita Krause
Marita Krause
Staff-Astronomer
Max-Planck-Institut für Radioastronomie
Auf dem Hügel 69
D-53121 Bonn
Tel: +49 228 525 312
Fax: +49 228 525 229
Email:mkrause at mpifr-bonn.mpg.de
RESEARCH INTERESTS:
Magnetic fields in disks and halos of spiral galaxies
Dynamo action and its observational signature
Origin and morphology of radio halos
Density waves and spiral structure
Morphology and dynamics of molecular gas in galaxies
Cold dust in galaxies
Physical conditions in the ISM in nearby galaxies
Radio - (far)infrared correlation in galaxies
Radio jets and their magnetic fields
My work is based on radio line-, continuum- and linear polarization- observations from submm to cm wavelength range with many different telescopes like the 100-m Effelsberg, VLA, Pico Veleta, Plateau de Bure Interferometer, Nobeyama 45-m and Millimeter Array, SEST and Heinrich-Hertz-Telescope.
Here you can get the program bfield.gz
to compute the strength of the total and regular magnetic fields from total and polarized synchrotron intensities as described by R.Beck & M.Krause, 2005, AN 326, No.6, 414. The program was compiled with SuSE linux 8.2.
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Last modified 19.01.2011
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