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SUMMARY:MHD Modes in the ISM: A Statistical Approach Using Synchrotron Pol
 arization
DTSTART:20260513T130000Z
DTEND:20260513T143000Z
DTSTAMP:20260622T093500Z
UID:indico-event-54@indico.iparcos.ucm.es
DESCRIPTION:Speakers: Parth Pavaskar (University of Potsdam & DESY Zeuthen
 )\n\nMagnetohydrodynamic (MHD) turbulence plays a fundamental role in shap
 ing the interstellar medium (ISM)\, influencing cosmic ray transport\, sta
 r formation\, and plasma dynamics.\nThe properties of the MHD turbulence a
 re governed by the energy fractions of the three fundamental plasma modes:
  the incompressible Alfvén\, and the compressible fast and slow modes. Ho
 wever\, identifying which mode dominates the energy remains a significant 
 observational challenge.\nI will present the modified Synchrotron Polariza
 tion Analysis (SPA+) method\, a technique to systematically identify the d
 ominant MHD mode in ISM plasma using synchrotron polarization observations
 \, helping us model the aforementioned processes better. I will further s
 how the application of this method to real observations\, analyzing the ma
 gnetized turbulence in the Cygnus loop region.\n\nhttps://indico.iparcos.u
 cm.es/event/54/
LOCATION:00.303.0 - Aula 13 (Facultad de Ciencias Físicas)
URL:https://indico.iparcos.ucm.es/event/54/
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