نتایج جستجو برای: ray spectrum

تعداد نتایج: 513243  

In this research zinc oxide (ZnO) nano-crystalline powders were prepared by sol-gel method using zinc acetate. The ZnO nanoparticles were characterized by X-ray diffraction (XRD), scanning electron microscopy (SEM), ultraviolet-visible (UV-Vis), Fourier transform infra-red (FT-IR) and energy dispersive X-ray (EDX) spectroscopy. The structure of nanoparticles was studied using XRD pattern. The c...

Journal: :international journal of nano dimension 0
g. narasimha applied microbiology laboratory, department of virology, sri venkateswara university, tirupati- 517502 andhra pradesh, india. b. praveen applied microbiology laboratory, department of virology, sri venkateswara university, tirupati- 517502 andhra pradesh, india. k. mallikarjuna department of physics, sri venkateswara university, tirupati-517502 andhra pradesh, india. b. deva prasad raju department of physics, sri venkateswara university, tirupati-517502 andhra pradesh, india.

in this paper we report an eco-friendly route for the synthesis of sliver nanoparticles using agaricus bisporus (white button mushroom) extract. the synthesized silver nanoparticles were confirmed and characterized by uv-visible spectrum of the aqueous solution containing silver ions showed a peak at 420 nm corresponding to the surface plasmon absorbance of silver nanoparticles. transmission el...

Journal: :Physical review letters 2013
F Albert B B Pollock J L Shaw K A Marsh J E Ralph Y-H Chen D Alessi A Pak C E Clayton S H Glenzer C Joshi

We present the first measurements of the angular dependence of the betatron x-ray spectrum produced by electrons inside the cavity of a laser-wakefield accelerator. Electrons accelerated up to 300 MeV energies produce a beam of broadband, forward-directed betatron x-ray radiation extending up to 80 keV. The angular resolved spectrum from an image plate-based spectrometer with differential filte...

Objective: The use of miniature X-ray source in electronic brachytherapy is on the rise so there is an urgent need to acquire more knowledge on X-ray spectrum production and distribution by a dose. The aim of this research was to investigate the influence of target thickness and geometry at the source of miniature X-ray tube on tube output.Method: Five sources were simulated based on problems e...

Journal: :Monthly Notices of the Royal Astronomical Society 1998

2007
C. DE DONATO G. A. MEDINA-TANCO

We use a diffusion galactic model to analyze the end of the Galactic cosmic ray spectrum and its mixing with the extragalactic cosmic ray flux. We analyze the transition between Galactic and extragalactic components using two different extragalactic models. We compare the sum of the diffusive galactic spectrum and extragalactic spectrum with the available experimental data.

2008
F. L. Villante F. Vissani

Supernova remnants are likely to be the accelerators of the galactic cosmic rays. Assuming the correctness of this hypothesis, we develop a method to extract the parent cosmic ray spectrum from the VHE gamma ray flux emitted by supernova remnants (and other gamma transparent sources). Namely, we calculate semi-analytically the (inverse) operator which relates an arbitrary gamma ray flux to the ...

Journal: :international journal of nano dimension 0
p. rejani nano science research lab, department of chemistry, d.b.college,sasthamcotta, kollam,kerala, india. a. radhakrishnan nano science research lab, department of chemistry, d.b.college,sasthamcotta, kollam,kerala, india. b. beena nano science research lab, department of chemistry, d.b.college,sasthamcotta, kollam,kerala, india.

zno nanorod was prepared by microwave assisted method. the crystal structure of the nano powders were confirmed by x-ray diffraction analysis and the mean particle size was estimated by the scherrer,s formula .the surface morphology of the nano particles were analyzed by   using sem . the absorption spectrum of the material in the uv-vis range was recorded .the energy band gap of the material w...

1996
P. Magdziarz A. A. Zdziarski

Analysis of broad-band X/γ-ray spectra of NGC 4151 shows that the data are well modelled with an intrinsic spectrum due to thermal Comptonization with temperature ∼ 50 keV and X-ray spectral index α ∼ 0.4– 0.7. The variable X-ray spectrum pivots at ∼ 100 keV, which is consistent with the observed approximatly constant γ-ray spectrum. The observed UV/X-ray correlation can be explained by two spe...

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