Observing the solar corona on the 11th of July 2012

Add to your list(s) Download to your calendar using vCal

• Dr. Stephane Regnier (UCLAN)
• Monday 10 February 2014, 16:00-17:00
• MR14, Centre for Mathematical Sciences, Wilberforce Road, Cambridge.

If you have a question about this talk, please contact Adrian Barker.

In the modern era of solar physics, we can continuously observe 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 from the Solar Dynamics Observatory (SDO) and Hi-C, I will describe new observations of the solar corona, including the nature and evolution of a unipolar streamer and sparkling EUV bright dots. I will discuss the importance of the coupling between the different spatial scales (from 100 km to 100 Mm) and the different time scales (from seconds to hours).

This talk is part of the DAMTP Astrophysics Seminars series.

This talk is included in these lists:

• All CMS events
• CMS Events
• Cambridge Astronomy Talks
• Cosmology, Astrophysics and General Relativity
• DAMTP Astrophysics Seminars
• DAMTP info aggregator
• Interested Talks
• MR14, Centre for Mathematical Sciences, Wilberforce Road, Cambridge
• bld31

Note that ex-directory lists are not shown.