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6篇 您的检索式：作者名="Karlicky M"

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		题名	作者	年代	出处	被引量
	1	Diagnosing physical conditions near the flare energy-release sites from observations of solar microwave typeⅢbursts显示文摘In the physics of solar flares, it is crucial to diagnose the physical conditions near the flare energyrelease 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.	Bao-Lin Tan Marian Karlicky Hana Mészárosová Guang-Li Huang	2016	Research in Astronomy and Astrophysics2016，16，5：	5
	2	Solar flare radio pulsations as a signature of dynamic magnetic reconnection 显示文摘	Kliem B Karlicky M Benz A O	2000	Astronomy and Astrophysics2000，360，2：	1
	3	Solar flare radio pulsations as a signature of dynamic magnetic reconnection 显示文摘	Kliem B Karlicky M Benz A O	2000	A&A2000，360，：	1
	4	Electron beam-plasma interaction and the return-current formation显示文摘	Karlicky M	2009	The Astrophysical Journal2009，690，1：	1
	5	High-frequency slowly drifting structures in solar flares 显示文摘	Karlicky M Farnik F Meszrosova H	2002	Astronomy and Astrophysics2002，395，2：	1
	6	Acceleration and heating processes in a collapsing magnetic trap 显示文摘	Karlicky M Kosugi T	2004	Astronomy and Astrophysics2004，419，3：	1

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