出版社：SISSA, Scuola Internazionale Superiore di Studi Avanzati
摘要：In the context of the new era of Cosmic Microwave Background Polarization
(CMBP) experiments, it is important to have reliable templates of the
polarized foregrounds contaminating the CMBP. This is specially true for the
for the Planck Surveyor Mission (ESA, 2007) and for the near-future B-mode
polarization probes. The Galactic Emission Mapping collaboration aims to
measure the polarization state and Stokes components at low frequencies (5-
10 Ghz) of the galactic synchrotron radiation using an antenna covering the
North Hemisphere and another the South Hemisphere. Together, the joint
coverage should produce a reliable template of the synchrotron polarization in
80% of the sky.
