Tan Baolin1; Marian Karlicky2; Hana Meszarosova2; Huang Guangli3
Source Publicationresearchinastronomyandastrophysics
AbstractIn the physics of solar flares, it is crucial to diagnose the physical conditions near the flare energy-release sites. However, so far it is unclear how to diagnose these physical conditions. A solar microwave type III burst is believed to be a sensitive signature of primary energy release and electron accelerations in solar flares. This work takes into account the effect of the magnetic field on the plasma density and develops a set of formulas which can be used to estimate the plasma density, temperature, magnetic field near the magnetic reconnection site and particle acceleration region, and the velocity and energy of electron beams. We apply these formulas to three groups of microwave type III pairs in an X-class flare, and obtained some reasonable and interesting results. This method can be applied to other microwave type III bursts to diagnose the physical conditions of source regions, and provide some basic information to understand the intrinsic nature and fundamental processes occurring near the flare energy-release sites.
Funding Project[National Natural Science Foundation of China] ; [MOST Grant] ; [National Major Scientific Equipment RD Project] ; [Astronomical Institute AS] ; [Marie Curie project]
Document Type期刊论文
2.Astronomical Institute of the Academy of Sciences of the Czech Republic
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Tan Baolin,Marian Karlicky,Hana Meszarosova,et al. diagnosingphysicalconditionsneartheflareenergyreleasesitesfromobservationsofsolarmicrowavetypeiiibursts[J]. researchinastronomyandastrophysics,2016,16(5).
APA Tan Baolin,Marian Karlicky,Hana Meszarosova,&Huang Guangli.(2016).diagnosingphysicalconditionsneartheflareenergyreleasesitesfromobservationsofsolarmicrowavetypeiiibursts.researchinastronomyandastrophysics,16(5).
MLA Tan Baolin,et al."diagnosingphysicalconditionsneartheflareenergyreleasesitesfromobservationsofsolarmicrowavetypeiiibursts".researchinastronomyandastrophysics 16.5(2016).
Files in This Item:
There are no files associated with this item.
Related Services
Recommend this item
Usage statistics
Export to Endnote
Google Scholar
Similar articles in Google Scholar
[Tan Baolin]'s Articles
[Marian Karlicky]'s Articles
[Hana Meszarosova]'s Articles
Baidu academic
Similar articles in Baidu academic
[Tan Baolin]'s Articles
[Marian Karlicky]'s Articles
[Hana Meszarosova]'s Articles
Bing Scholar
Similar articles in Bing Scholar
[Tan Baolin]'s Articles
[Marian Karlicky]'s Articles
[Hana Meszarosova]'s Articles
Terms of Use
No data!
Social Bookmark/Share
All comments (0)
No comment.

Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.