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SUMMARY:Observing the solar corona on the 11th of July 2012 - Dr. Stephane
  Regnier (UCLAN)
DTSTART:20140210T160000Z
DTEND:20140210T170000Z
UID:TALK49779@talks.cam.ac.uk
CONTACT:Adrian Barker
DESCRIPTION:In the modern era of solar physics\, we can continuously obser
 ve the solar corona at high time cadence and high spatial resolution in a 
 broad range of wavelengths from X-rays to radio. Based on observations fro
 m the Solar Dynamics Observatory (SDO) and Hi-C\, I will describe new obse
 rvations of the solar corona\, including the nature and evolution of a uni
 polar streamer and sparkling EUV bright dots. I will discuss the importanc
 e of the coupling between the different spatial scales (from 100 km to 100
  Mm) and the different time scales (from seconds to hours). 
LOCATION:MR14\,  Centre for Mathematical Sciences\, Wilberforce Road\, Cam
 bridge
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