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SUMMARY:The polarizing puzzle of dusty disks
DTSTART;VALUE=DATE-TIME:20200512T140000Z
DTEND;VALUE=DATE-TIME:20200512T142000Z
DTSTAMP;VALUE=DATE-TIME:20240704T115618Z
UID:indico-contribution-10@meetings.aip.de
DESCRIPTION:Speakers: Gesa H.-M. Bertrang (MPIA)\nFrom a theoretical point
 -of-view\, magnetic fields are crucial to the evolution of planet-forming 
 disks. However\, profound observational constraints are pending. Presently
 \, the number of cutting-edge polarization observations presenting inconcl
 usive data increases continuously. In very recent years\, polarization at 
 mm-wavelengths\, the classical tracer of magnetic fields\, emerged as high
 ly ambiguous\, and the pressing demand for comprehensive tools to analyze 
 these new observations is growing.\n\nI will present an overview on the so
 urces of continuum polarization with focus on the impact of grain alignmen
 t\, scattering\, and grain porosity on the polarization measurement – as
  well as a potential solution to this dusty ambiguousness\, linearly polar
 ized gas emission.\n\nhttps://meetings.aip.de/event/1/contributions/10/
LOCATION:Leibniz Institute for Astrophysics Potsdam (AIP) Lecture Hall
URL:https://meetings.aip.de/event/1/contributions/10/
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