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SUMMARY:Modeling of the solar chromosphere
DTSTART;VALUE=DATE-TIME:20230509T120000Z
DTEND;VALUE=DATE-TIME:20230509T122500Z
DTSTAMP;VALUE=DATE-TIME:20240704T115653Z
UID:indico-contribution-357@meetings.aip.de
DESCRIPTION:Speakers: Sanja Danilovic (Sanja)\nThe chromosphere is a dynam
 ic and complex layer where all the relevant physical processes happen on v
 ery small spatio-temporal scales. A few spectral lines that can be used as
  chromospheric diagnostics\, give us convoluted information that is hard t
 o interpret without realistic theoretical models. What are the key ingredi
 ents that these models need to contain? In this review\, we present the re
 cent numerical models and how they compare to observations. We will discus
 s the formation and properties of chromospheric structures at different sp
 atial scales and the challenges we meet when modeling the solar chromosphe
 re.\n\nhttps://meetings.aip.de/event/24/contributions/357/
LOCATION:Haus H\, Telegrafenberg
URL:https://meetings.aip.de/event/24/contributions/357/
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