Observing the solar corona on the 11th of July 2012
- š¤ Speaker: Dr. Stephane Regnier (UCLAN)
- š Date & Time: Monday 10 February 2014, 16:00 - 17:00
- š Venue: MR14, Centre for Mathematical Sciences, Wilberforce Road, Cambridge
Abstract
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).
Series This talk is part of the DAMTP Astrophysics Seminars series.
Included in Lists
- All CMS events
- bld31
- Cambridge Astronomy Talks
- CMS Events
- Cosmology, Astrophysics and General Relativity
- DAMTP Astrophysics Seminars
- DAMTP info aggregator
- Interested Talks
- MR14, Centre for Mathematical Sciences, Wilberforce Road, Cambridge
Note: Ex-directory lists are not shown.
![[Talks.cam]](/static/images/talkslogosmall.gif)

Dr. Stephane Regnier (UCLAN)
Monday 10 February 2014, 16:00-17:00