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Abstract Stellar scintillations observed from space through the atmosphere show that density inhomogeneities in the stratosphere are stretched along the Earth's surface. This is true for vertical scales above dozens of metres. The observations reveal the existence of locally isotropic small-scale structure with fluctuation sizes up to fractions of a metre. The subject of this paper is to find out how the rotation of inhomogeneities with respect to the passing ray affects scintillations. Another subject of this study is chromatic aberration in the atmosphere which distorts the scintillation spectra. Numerical modelling within the weak-fluctuation approximation showed that the characteristic value of the anisotropy parameter is equal to the square root of the Earth's radius divided by the atmospheric scale. After the anisotropy exceeds this value, the growth of scintillation variance quickly becomes saturated. Chromatic aberration suppresses the high-frequency branch of the scintillation spectrum. However, information on the structure of isotropic fluctuations with scales up to the Fresnel radius is retained in scintillation spectra for oblique occultations. The model of composing blocks is suggested to develop the approximation for a three-dimensional fluctuation spectrum in the stratosphere. Parameters of these blocks can be determined from the set of measured scintillation spectra. 相似文献
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V. Brekhovskikh A. Gorin V. Dyatchenko M. Medynsky V. Rykalin 《Physics of Atomic Nuclei》2019,82(6):649-656
The work is dedicated to the discussion of four new types of large-area scintillation counters design intended for detection of EAS and the use in the guard systems of experimental physics setups with low-cost production. The solid counters based on scintillating polystyrene plates are produced by melting clear polystyrene granules with additives in a mirror mold. Other counters are based on lentil-like polystyrene scintillation granules which are a new kind of plastic scintillators produced at IHEP. WLS fibers and SiPM as a photo sensor are used for a light detection. The dimensions of the tested detectors were 500 × 500 and to 1000 × 1000 mm2, their measured light output was up to 180 ph.e. 相似文献
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Burtovoy V. S. Akimenko S. A. Artamonov A. V. Blik A. M. Brekhovskikh V. V. Gorin A. M. Donskov S. V. Inyakin A. V. Kolosov V. N. Kurshetsov V. F. Lishin V. A. Medynsky M. V. Mikhailov Yu. V. Obraztsov V. F. Polyakov V. A. Romanovsky V. I. Rykalin V. I. Sadovsky A. S. Samoilenko V. D. Stenyakin O. V. Uvarov V. A. Filin A. P. Khaustov G. V. Kholodenko S. A. Tchikilev O. G. Yushchenko O. P. Guschin E. N. Duk V. A. Kravtsov V. I. Kudenko Yu. G. Polyarush A. Yu. Filippov S. N. Khudyakov A. A. Bychkov V. N. Zalikhanov B. Zh. Kekelidze G. D. Lysan V. M. 《Journal of Experimental and Theoretical Physics》2020,131(6):928-939
Journal of Experimental and Theoretical Physics - On the statistics of ~1.7 × 108 interactions of positively charged kaons on copper nuclei, coherent events of the K+π0 system production... 相似文献
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G.L. Brekhovskikh V.V. Zverev N.Y. Okladnikov A.I. Sokolovskaia 《Optics Communications》1985,53(1):59-63
The energy dependence and the total saturation of the SRS and SBS are investigated in the nanosecond range at different geometries of the illuminated volume. The theoretical explanation of the experimental results for SRS is given, the change of the vibrational level population being taken into account. The solution of the quasi-stationary equations for SRS if shown to have the form of a solitary wave. The results of the work permit to govern the amplitude-phase distribution of the complex light fields at the stimulated scatterings. 相似文献