Diagnosing physical conditions near the flare energy-release sites from observations of solar microwave type III bursts

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F16%3A00462794" target="_blank" >RIV/67985815:_____/16:00462794 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1088/1674-4527/16/5/082" target="_blank" >http://dx.doi.org/10.1088/1674-4527/16/5/082</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1088/1674-4527/16/5/082" target="_blank" >10.1088/1674-4527/16/5/082</a>

Result language
angličtina
Original language name
Diagnosing physical conditions near the flare energy-release sites from observations of solar microwave type III bursts
Original language description
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 re
Czech name
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Czech description
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Type
J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Project
<a href="/en/project/GAP209%2F12%2F0103" target="_blank" >GAP209/12/0103: Radio and X-ray diagnostics of primary-energy-release processes in solar flares and their numerical simulations</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2016
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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