Distribution for the Regular Component of the Galactic Magnetic Field Using 5-Year WMAP Data
We have studied the spatial structure of the three dimensional large-scale pattern of the Galactic Magnetic Field using the polarization maps obtained by the WMAP satellite at 22 GHz. By using different models of the large-scale magnetic field of the Milky Way and a certain model for the cosmic rays electron distribution, we predict the expected
Ruiz-Granados, B. et al.
Fecha de publicación:
2010