Spectroscopic Detection of Magnetic Reconnection Evidence in the Solar Atmosphere with SolarB/EIS

Physics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

1

Scientific paper

2.5D MHD simulations of CMEs and flares are combined with improved accuracy density sensitive line emission contribution functions from the ADAS database to study profiles of spectral lines which will fall within the wavelength range of the SolarB Extreme ultraviolet Imaging Spectrometer (EIS). The objective is to study the signatures of magnetic reconnection associated flow phenomena in the line profiles and provide a set of recommended lines for EIS observations planning. Here, we illustrate our methods by considering the profile of the well-known Ion{Fe{XII}} 195 AA line and its ability to detect reconnection inflows. We also discuss the effects of altering simulation parameters such as electron temperature and the inclusion of the effect of heat conduction. The table of recommended lines following these methods is being prepared and will be presented in a separate paper.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Spectroscopic Detection of Magnetic Reconnection Evidence in the Solar Atmosphere with SolarB/EIS does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Spectroscopic Detection of Magnetic Reconnection Evidence in the Solar Atmosphere with SolarB/EIS, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectroscopic Detection of Magnetic Reconnection Evidence in the Solar Atmosphere with SolarB/EIS will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1023286

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.