Surcis, GabrieleGabrieleSurcisVlemmings, Wouter H. T.Wouter H. T.VlemmingsLankhaar, BoyBoyLankhaarvan Langevelde, Huib JanHuib Janvan Langevelde2020-10-132020-10-132018978-11071924541743-9213http://hdl.handle.net/20.500.12386/27765Through the observations and the analysis of maser polarization it is possible to measure the magnetic field in several astrophysical environments (e.g., star-forming regions, evolved stars). In particular from the linearly and circularly polarized emissions we can determine the orientation and the strength of the magnetic field, respectively. In these proceedings the implications, on observed data, of the new estimation of the Landé g-factors for the CH<SUB>3</SUB>OH maser are presented. Furthermore, some example of the most recent results achieved in observing the polarized maser emission from several maser species will also be reported.STAMPAenConference paper10.1017/S17439213170116322-s2.0-85060083651https://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/maser-polarization/BA5256FF2ADF7E35FD59AB1AEC4E039D2018IAUS..336...27SFIS/05 - ASTRONOMIA E ASTROFISICAERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation