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|  | | 为了更好的帮助您理解掌握查询词或其译词在地道英语中的实际用法,我们为您准备了出自英文原文的大量英语例句,供您参考。 | |
Finite energy band-limited functions are reconstructed iteratively
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We also report the time profiles of the flare of October 29, 2003, in the energy bands corresponding to the continuum in the energy band 0.3-0.6 MeV, the nuclear lines of 56Fe, 24Mg, 20Ne, 28Si, 12C, and 16O, and the 2.2-MeV neutron-capture line.
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We present data on the Spin-X sensitivity achievable during long-term observations of persistent and transient sources and on its sensitivity to X-ray bursts from Galactic sources in the 2-30-keV energy band.
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The SIGMA telescope recorded relatively bright bursts with peak fluxes of 10-6-10-4 erg s-1 cm-2 in the 100-500-keV energy band.
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XMM-Newton yields an upper limit on the SNR luminosity in the 2-10 keV energy band, LX ? 5 × 1034 erg s-1.
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Frequency-Domain Bounds for Nonnegative, Unsharply Band-Limited Functions
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Aliasing error bounds are derived for one- and two-channel sampling series analogous to the Whittaker-Kotel'nikov-Shannon series, and for the multi-band sampling series, and a "derivative" extension of it, due to Dodson, Beaty, et al.
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In this paper we give a further investigation of the method introduced by the author in [1, Frequency-domain bounds for nonnegative unsharply band-limited functions] for proving bounds for functions with nonnegative Fourier transforms.
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Finite energy band-limited functions are reconstructed iteratively
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Unique reconstruction of band-limited signals by a Mallat-Zhong wavelet transform algorithm
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We also report the time profiles of the flare of October 29, 2003, in the energy bands corresponding to the continuum in the energy band 0.3-0.6 MeV, the nuclear lines of 56Fe, 24Mg, 20Ne, 28Si, 12C, and 16O, and the 2.2-MeV neutron-capture line.
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Analysis of the soft X-ray emission in two energy bands detected by the GOES satellites for about 20 powerful solar flares reveals long time intervals during the decay phase when the source temperature decreases, in general, exponentially.
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The paper considers the topological characteristics of dispersion functions ?s(p) in energy bands in single crystals related to classical electron trajectories in uniform magnetic fields.
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The two-orbital Hubbard model is used to obtain formulas for the fermion excitation spectrum in the energy bands hybridized by the Anderson interaction.
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An attempt is made to calculate the energy bands and spectra of the characteristic CKα emission of small-diameter carbon nanotubes.
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Since the discovery of CNTs, people have employed more serious quantum mechanical methods, including the electronic band theory, tight-binding theory, scattering theory and density function theory, to investigate FE of CNTs.
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LMTO calculations of the electronic band structure showed that CaCo2 forms as a result of an s-d electronic transition of Ca and in the ground state it is a ferromagnet with a high magnetic moment per Co atom.
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The electronic band structure of corundum (α-Al2O3) is calculated by the ab initio density functional method and compared with experimental results.
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However, it is less demanding to the quality of experimental data and makes it possible to study situations where only a portion of the electronic band profile is accessible for analysis.
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Specific features of magnetoabsorption resulting from exactly taking into account the electronic band spectrum
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