Quantitative spectral radiation measurements in the VUV and soft X-ray region

1996 ◽  
Vol 28 (3) ◽  
pp. 299-307 ◽  
Author(s):  
G. Ulm ◽  
B. Wende
2019 ◽  
Vol 185 (2) ◽  
pp. 157-167
Author(s):  
R Behrens ◽  
M Reginatto

AbstractSpectrum deconvolution is an important task in ionizing radiation measurements, as the pulse height spectra, or, in general, the measured data from spectrometers or other measuring instruments are usually determined by the convolution of the response function with the fluence spectra. The method presented here for obtaining fluence spectra from the measurements is an application of Bayesian parameter estimation to the deconvolution of X-ray emission data. The problem of choosing the optimal model among several possible models is also considered, as well as an approach to include contributions from various sources of uncertainty, both correlated and uncorrelated. The application is carried out using the Bayesian software WinBUGS.


2019 ◽  
Vol 2019 ◽  
pp. 1-20 ◽  
Author(s):  
Mohammed Benchrifa ◽  
Hajar Essalhi ◽  
Rachid Tadili ◽  
Mohammed N. Bargach ◽  
Abdellah Mechaqrane

The main objective of this work is to create a daily updated database that includes all components of solar radiation, either energetic or spectral radiation. This will lead us to quantify the Moroccan solar potential and to determine the dimensions of all types of solar thermal and photovoltaic systems. Consequently, the obtained database will be the fundamental support for engineers, designers, and all organizations interested in developing solar systems, in different regions throughout Morocco. It will also be a basic tool for researchers in modelling and simulating the new solar systems. Firstly, we used one year’s worth of measurements of the different components of the solar radiation, provided by the National Meteorological Department, to establish the extrapolation equations between the global radiation at the reference site and the global radiation of twenty-eight other sites. As well as with the same measurements, we developed the correlation equations between the global solar radiation and the other solar radiation components. Secondly, from ten years of Fez station’s daily global radiation measurements and through the extrapolation equations, we were able to estimate the global radiation of all Moroccan cities. Then, by using the obtained global radiation data and the correlation equations, we predicted the other components of solar radiation. Subsequently, with a new measurement campaign carried out on several sites, we validated the estimation models by using the usual statistical indicators. In addition, we compared our results with those obtained by other estimation models. The resulting differences for each solar component display the advantage of our model with errors under 6%. To facilitate the use of our results, we compiled them into maps representing the spread of solar radiation across Morocco.


2021 ◽  
Vol 11 (23) ◽  
pp. 11574
Author(s):  
Vladimir A. Srećković ◽  
Desanka M. Šulić ◽  
Veljko Vujčić ◽  
Zoran R. Mijić ◽  
Ljubinko M. Ignjatović

Strong radiation from solar X-ray flares can produce increased ionization in the terrestrial D-region and change its structure. Moreover, extreme solar radiation in X-spectral range can create sudden ionospheric disturbances and can consequently affect devices on the terrain as well as signals from satellites and presumably cause numerous uncontrollable catastrophic events. One of the techniques for detection and analysis of solar flares is studying the variations in time of specific spectral lines. The aim of this work is to present our study of solar X-ray flare effects on D-region using very low-frequency radio signal measurements over a long path in parallel with the analysis of X-spectral radiation, and to obtain the atmospheric parameters (sharpness, reflection height, time delay). We introduce a novel modelling approach and give D-region coefficients needed for modelling this medium, as well as a simple expression for electron density of lower ionosphere plasmas. We provide the analysis and software on GitHub.


1991 ◽  
Vol 230 ◽  
Author(s):  
Roy Clarke ◽  
Waldemar Dos Passos ◽  
Walter Lowe ◽  
Brian Rodricks ◽  
Cristine Brizard

AbstractA new time-resolved x-ray method of probing the kinetics of interfacial strains in semiconductor heterostructures is presented. High-resolution synchrotron radiation measurements of the strain relaxation during rapid thermal annealing (RTA) show that the lattice strain of an as-grown strained layer structure GaAs-Inx.Ga1−x-As-GaAs/GaAs is relieved cooperatively by a series of sluggish discontinuous transitions. We find that ion implantation enhances the annealing kinetics of InAlAs strained layers.


1975 ◽  
Vol 51 (4) ◽  
pp. 249-250 ◽  
Author(s):  
G.I. Brukhnevitch ◽  
V.K. Chevokin ◽  
Yu.S. Kasyanov ◽  
V.V. Korobkin ◽  
A.A. Malyutin ◽  
...  

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