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BEGIN:VEVENT
DTSTAMP:20260519T164909Z
DTSTART;VALUE=DATE-TIME:20200316T150000
DTEND;VALUE=DATE-TIME:20200316T160000
SUMMARY:Dominik Utz (University of Graz): Small-scale solar magnetic fiel
 ds as seen by MBPs: From quiet-sun basics over activity to coronal holes
  - CANCELLED!
TZID:Europe/London
UID:20200316-8a1785d86fb3493d016fc257f2f31322@warwick.ac.uk
CREATED:20200313T142411Z
DESCRIPTION:Author: Dominik Utz Affiliation: IGAM/Institute of Physics\, 
 University of Graz\, Austria\; Instituto de Astrofísica de Andalucía IAA
 -CSIC\, Granada\, Spain Title: Small-scale solar magnetic fields as seen
  by MBPs: From quiet-sun basics over activity to coronal holes Abstract:
  The Sun is our host star and not at all a dull ball of gas\, but instea
 d an impressive heavenly body\, due to its activity within its atmospher
 e. All of this activity is caused by magnetic fields\, which range from 
 gigantic active regions - consisiting of sunspots or even sunspot groups
  - down to isolated single flux fibres\, often visible as magnetic brigh
 t points (MBPs). While sunspots are very important to understand the glo
 bal solar magnetic field dynamo\, as well as the caused large scale-sola
 r activity\, and hence the space weather and its influence on Earth\, sm
 all-scale solar magnetic fields can teach us about important magneto-pla
 sma processes such as MHD wave generation and propagatin. In this sminar
 y talk\, we wish to shed light on MBPs\, which are due to their size amo
 ng the smallest solar magnetic feastures we can study currently and thus
  of great importance to advance the field. Moreover\, they have the adva
 ntage that identifying them in "simple" filtergram images\, is of an eas
 ier and especially faster task than analysing cumbersome and low cadence
  spectro-polarimetric data. We will outline first of all the basic chara
 cterstics of MBPs\, then have a look in solar-activity processes they ar
 e involved in such as magnetic reconnection and MHD wave creation and pr
 opagation\, before touching shortly large scale-structures - namely coro
 nal holes - and their relationship to MBPs.
LOCATION:PS128
CATEGORIES:CFSA Seminar
LAST-MODIFIED:20200313T142411Z
ORGANIZER;CN=Anne-Marie Broomhall:
END:VEVENT
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