Hard X-ray characteristics of solar flares using electron Monte-Carlo calculations and beamed thick target model

Rausaria, R. R

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dc.contributor.author	Rausaria, R. R
dc.date.accessioned	2008-06-26T09:11:58Z
dc.date.available	2008-06-26T09:11:58Z
dc.date.issued	1992-08
dc.identifier.citation	Astrophysics and Space Science, Vol. 194, No. 2, pp. 261 - 301	en
dc.identifier.issn	0004-640X (Print) 1572-946X (Online)
dc.identifier.uri	http://hdl.handle.net/2248/2509
dc.description.abstract	The experimental results of X-ray bursts with spectral characteristics, spatial distribution, fast time variations, polarization, and directivity measurements carried out with Intercosmos, PVO/ISEE-3 spacecrafts, imaging instrument observations of Hard X-ray (HXIS) and Hard X-ray Burst Spectrometers (HXRBS) during solar maximum mission have been reviewed. The observed results about the above characteristics are discussed in detail in terms of non-thermal and thermal models. It is shown that the results can be interpreted in terms of beamed thick-target model in which electrons stream down to the loop footpoints and produce hard X-rays through electron-ion bremsstrahlung	en
dc.format.extent	3350134 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Springer Netherlands	en
dc.relation.uri	http://www.springerlink.com/content/k05gk022m341t215/	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1992Ap%26SS.194..261R	en
dc.subject	BREMSSTRAHLUNG	en
dc.subject	MONTE CARLO METHOD	en
dc.subject	SOLAR ATMOSPHERE	en
dc.subject	SOLAR FLARES	en
dc.subject	SOLAR X-RAYS	en
dc.subject	ELECTRON DISTRIBUTION	en
dc.subject	ENERGY SPECTRA	en
dc.subject	PLASMA DENSITY	en
dc.subject	X RAY SPECTRA	en
dc.title	Hard X-ray characteristics of solar flares using electron Monte-Carlo calculations and beamed thick target model	en
dc.type	Article	en