Sturm und Drang: The turbulent, magnetic tempest in the Galactic center

"New Trends in the Form and Function of the Dénouement: German Empfindsamkeit and Sturm und Drang"

Turbulent Origin of the Galactic-Center Magnetic Field: Nonthermal Radio Filaments

A great deal of study has been carried out over the last twenty years on the origin of the magnetic activity in the Galactic center. One of the most popular hypotheses assumes milli-Gauss magnetic field with poloidal geometry, pervading the inner few hundred parsecs of the Galactic-center region. However, there is a growing observational evidence for the large-scale distribution of a much weake...

Can the turbulent galactic dynamo generate large - scale magnetic fields ?

Large-scale magnetic fields in galaxies are thought to be generated by a turbulent dynamo. However the same turbulence also leads to a small-scale dynamo which generates magnetic noise at a more rapid rate. The efficiency of the large-scale dynamo depends on how this noise saturates. We examine this issue taking into account ambipolar drift, which obtains in a galaxy with significant neutral ga...

Interstellar magnetic fields in the Galactic center region

Aims. We seek to obtain a picture of the interstellar magnetic field in the Galactic center region that is as clear and complete as

the u.s. policy in central asia and its impact on the colored revolutions in the region (the case study of tulip revolution in kyrgyzstan)

چکیده ندارد.