PMO OpenIR
diagnosingphysicalconditionsneartheflareenergyreleasesitesfromobservationsofsolarmicrowavetypeiiibursts
Tan Baolin1; Marian Karlicky2; Hana Meszarosova2; Huang Guangli3
2016
Source Publicationresearchinastronomyandastrophysics
ISSN1674-4527
Volume16Issue:5
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.
Language英语
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/30984
Collection中国科学院紫金山天文台
Affiliation1.中国科学院国家天文台
2.Astronomical Institute of the Academy of Sciences of the Czech Republic
3.中国科学院紫金山天文台
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).
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