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SUMMARY:Changes in the Lower Solar Atmosphere throughout the Solar Cycle
DTSTART;VALUE=DATE-TIME:20230512T070000Z
DTEND;VALUE=DATE-TIME:20230512T071500Z
DTSTAMP;VALUE=DATE-TIME:20240704T115653Z
UID:indico-contribution-344@meetings.aip.de
DESCRIPTION:Speakers: James Crowley (National Solar Observatory\; Universi
 ty of Colorado\, Boulder)\nThe change in the distribution of the magnetic 
 field in the quiet Sun photosphere over the solar cycle could be expected 
 to cause systematic variations in the photospheric thermodynamic structure
 . This could be due to changes in the dynamics of the convective overshoot
  or radiative properties. To look for such changes\, we use high spatial a
 nd spectral resolution spectropolarimetric observations obtained by Hinode
  SOT and apply the Spectropolarimetric Inversions Based on Response Functi
 ons (SIR) code to infer physical conditions in the lower solar photosphere
 . By using multiple homogeneous datasets acquired over 15 years\, we analy
 ze the distributions of the inferred parameters in the granules and interg
 ranules of magnetic and non-magnetic spectra throughout the solar cycle. T
 he final goal of our study is to characterize changes in the inferred atmo
 spheric parameters\, notably\, the temperature structure\, the line-of-sig
 ht velocities\, and magnetic properties.\n\nhttps://meetings.aip.de/event/
 24/contributions/344/
LOCATION:Haus H\, Telegrafenberg
URL:https://meetings.aip.de/event/24/contributions/344/
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