BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//Erlangen Centre for Astroparticle Physics - ECPv6.2.3.2//NONSGML v1.0//EN
CALSCALE:GREGORIAN
METHOD:PUBLISH
X-WR-CALNAME:Erlangen Centre for Astroparticle Physics
X-ORIGINAL-URL:https://ecap.nat.fau.de
X-WR-CALDESC:Events for Erlangen Centre for Astroparticle Physics
REFRESH-INTERVAL;VALUE=DURATION:PT1H
X-Robots-Tag:noindex
X-PUBLISHED-TTL:PT1H
BEGIN:VTIMEZONE
TZID:Europe/Berlin
BEGIN:DAYLIGHT
TZOFFSETFROM:+0100
TZOFFSETTO:+0200
TZNAME:CEST
DTSTART:20190331T010000
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:+0200
TZOFFSETTO:+0100
TZNAME:CET
DTSTART:20191027T010000
END:STANDARD
END:VTIMEZONE
BEGIN:VEVENT
DTSTART;TZID=Europe/Berlin:20190207T120000
DTEND;TZID=Europe/Berlin:20190207T130000
DTSTAMP:20260419T062407
CREATED:20181004T132210Z
LAST-MODIFIED:20181004T132210Z
UID:2466-1549540800-1549544400@ecap.nat.fau.de
SUMMARY:ECAP Seminar: Marijke Haverkorn
DESCRIPTION:The Magnetic Field of the Milky Way\nThe Milky Way’s magnetic field has coherent structures on Galactic scales\, following spiral arms but also Galactic outflows. It also has a turbulent component\, which influences the galactic ecosystem in many ways\, such as delaying star formation\, isotropizing Galactic cosmic rays\, and providing significant pressure component. \nThese magnetic field components can only be detected indirectly\, through the signature they leave on various kinds of radiation and particles\, observations of which are fitted to models of the Galactic magnetic field. Traditionally\, radio polarimetry is most used to probe Galactic magnetic fields\, with radio detectors in frequency ranges from LOFAR to Planck giving unique information. \nI will discuss some of the recent progress in this field\, and our new project called IMAGINE\, which aims to combine all different observational tracers and prior information to build a next-generation model of the Galactic magnetic field.
URL:https://ecap.nat.fau.de/index.php/event/ecap-seminar-marijke-haverkorn/
LOCATION:ECAP\, room 307\, Erwin-Rommel-Str 1\, Erlangen\, 91058\, Germany
CATEGORIES:Seminar
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Berlin:20190214T120000
DTEND;TZID=Europe/Berlin:20190214T130000
DTSTAMP:20260419T062407
CREATED:20190130T085139Z
LAST-MODIFIED:20190130T085139Z
UID:2624-1550145600-1550149200@ecap.nat.fau.de
SUMMARY:ECAP Seminar: Takaaki Tanaka
DESCRIPTION:Recent Results from X-ray Studies of Supernova Remnants\nX-ray emission from supernova remnants provides us with probes to high energy phenomena such as acceleration of cosmic-ray particles and nucleosynthesis in supernova explosions. In this talk\, I will present some of recent results that I\, with my students and collaborators\, obtained from observations with Suzaku\, Chandra\, XMM-Newton\, and NuSTAR satellites. I will mainly cover results related to particle acceleration and over-ionized plasma in Galactic supernova remnants. I will also talk about expectations brought about by high resolution spectroscopy with future X-ray observatories such as XRISM\, which is scheduled to be launched in 2021.
URL:https://ecap.nat.fau.de/index.php/event/ecap-seminar-takaaki-tanaka/
LOCATION:ECAP\, room 307\, Erwin-Rommel-Str 1\, Erlangen\, 91058\, Germany
CATEGORIES:Seminar
END:VEVENT
END:VCALENDAR