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搜索结果: 1-15 共查到理学 Hard X-Ray相关记录17条 . 查询时间(0.094 秒)
Advances continue to be made in hard x-ray, gamma-ray, neutron detectors and associated technologies for spectroscopy and imaging of these energetic photons and particles. Many types of position and e...
2017SPIE硬X射线,伽玛射线和中子探测器物理专题会议(Hard X-Ray,Gamma-Ray,and Neutron Detector Physics XIX)。
Hard X-Ray, Gamma-Ray, and Neutron Detector Physics XVIII     Hard X-Ray  Gamma-Ray       font style='font-size:12px;'> 2016/7/28
Breakthrough energy resolution, R(662keV) <4%, has been achieved with a transparent ceramic oxide scintillator, Cerium-doped Gadolinium Yttrium Gallium Aluminum Garnet, or GYGAG(Ce), by optimizing fab...
Gigahertz (GHz) imaging using hard X-rays ($\gtrsim$ 10 keV) can be useful to high-temperature plasma experiments, as well as research using coherent photons from synchrotron radiation and X-ray free ...
Improvements of in-orbit calibration of GSO scintillators in the Hard X-ray Detector on board Suzaku are reported. To resolve an apparent change of the energy scale of GSO which appeared across the la...
We report Fermi/LAT observations and broad-band spectral modeling of the radio-loud active galaxy 4C +55.17 (z=0.896), formally classified as a flat-spectrum radio quasar. Using 19 months of all-sky s...
We have assembled the largest sample of ultra hard X-ray selected (14-195 keV) AGN with host galaxy optical data to date, with 185 nearby (z<0.05), moderate luminosity AGN from the Swift BAT sample. T...
Over the last few years there has been much interest in the production of hard X-rays from various targets using a kHz short pulse laser at intensities above 1014Wcm-2 (A). Most of these studies have ...
The influence of albedo on the size of hard X-ray flare sources     albedo  hard X-ray        font style='font-size:12px;'> 2011/1/11
Context: Hard X-rays from solar flares are an important diagnostic of particle acceleration and transport in the solar atmosphere. Any observed X-ray flux from on-disc sources is composed of direct em...
Context. Extragalactic nuclear activity is best explored with observations at high energies, where the most extreme flux and spectral variations are expected to occur, witnessing changes in the accret...
The origin of the diffuse hard X-ray emission of starburst galaxies is a long-standing problem. We suggest that synchrotron emission of 10 - 100 TeV electrons and positrons can contribute significantl...
This article reports development of a practical laboratory hard X-ray photoelectron spectroscopy (HXPS) system by combining a focused monochromatic Cr X-ray source, a wide angle acceptance objectiv...
Infrared Hunting for New Hidden Hard X-ray Sources:Observations and Instrumentation。
The nature of the compact object in the hard x-ray Source 4u2206+54     hard x-ray  Source 4u2206+54       font style='font-size:12px;'> 2009/6/17
The nature of the compact object in the hard x-ray Source 4u2206+54。
Morphology and Spectral Behavior of Solar Hard X-Ray Sources     Solar Hard X-Ray  Morphology       font style='font-size:12px;'> 2009/6/11
Morphology and Spectral Behavior of Solar Hard X-Ray Sources。

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