BEGIN:VCALENDAR
VERSION:2.0
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METHOD:PUBLISH
BEGIN:VEVENT
DTSTART;TZID=Atlantic/Canary:20091111T000000
DTEND;TZID=Atlantic/Canary:20091111T010000
UID:iactalks-166
X-WR-CALNAME: IAC Talks: Open Astronomy Seminars
X-ORIGINAL-URL: /iactalks/Talks/view/166
CREATED:2009-11-11T00:00:00+00:00
X-WR-CALDESC: IAC Talks upcomming talks
SUMMARY:Response of the solar atmosphere to the photospheric plasma motion
DESCRIPTION:Response of the solar atmosphere to the photospheric plasma mot
 ion\nDr. Jörg Büchner\n\nThe dynamics of the solar atmosphere is largely
  controlled by its magnetic coupling to the photosphere of the Sun. Since 
 the solar magnetic field is complex, numerical simulation must be utilized
  to investigate the coupling processes. Results will be shown of treating 
 this way the two unresolved issues - the heating of the corona and the acc
 eleration of the solar wind.
END:VEVENT
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