Search engine for discovering works of Art, research articles, and books related to Art and Culture
ShareThis
Javascript must be enabled to continue!

Multiple scattering and attenuation for electromagnetic wave propagation in sand and dust atmosphere

View through CrossRef
For an electronic system operation under the conditions of all-weather in arid and semiarid areas, the studies of the attenuation and multiple scattering are necessary for electromagnetic wave propagations in sand and dust atmosphere. Based on Mie theory, a method of calculating the attenuations for electromagnetic wave propagation through sand and dust atmosphere is presented in this paper, which relate to the particle size distributions and visibilities for sand and dust atmosphere. The attenuations at 37 GHz are given for various visibilities, and are compared with the results calculated from other formulas and the experimental data from the literature. The attenuations are closer to the experimental results. In order to investigate into electromagnetic wave propagations in lower visibility sand and dust atmosphere, the multiple scattering in sand and dust storms are necessarily analyzed. At 37 and 93 GHz, the extinction cross sections, albedos and asymmetry factors are calculated by Mie theory for various size sand and dust particles. By the Monte Carlo (MC) simulation method, the attenuations for including the multiple scattering effects are calculated under the conditions of dry and 5% water content in sand and dust particles, respectively, and are compared with the results from Mie theory. The results are shown that the difference between the attenuation obtained by Mie and that by MC is small at 37 GHz. The influence of the multiple scattering on attenuation is small and may be ignored at 37 GHz. At 93 GHz, the difference between the attenuation obtained by Mie and that by MC is clear, and the attenuation obtained by using Mc simulation is smaller than that based on Mie theory. The effect of the multiple scattering on attenuation is evident at 93 GHz. The lower the visibility, the more notable the effect on attenuation is. For different sand and dust storms, the particle refractive indexes and the particle size distributions are different. For the sand and dust storms in Tengger desert and the blowing sand and dust atmosphere in north China, the attenuations at 93 GHz are analysed. In Tengger desert, the attenuation and the multiple scattering are larger than in blowing sand and dust atmosphere. The results show that the more the large size particles in sand and dust storms, the stronger the effect multiple scattering on attenuation is. Hence, for stronger sand and dust storms, the attenuation and the effect of multiple scattering become important. With the increase of water content in particle, the imaginary part of refractive index increases, the attenuation greatly increases, and the effect of the multiple scattering on attenuation is weakly varied. The analyses show that the attenuations for electromagnetic wave propagation in arid sand and dust atmosphere are smaller than in moisture sand and dust atmosphere under the condition of the same visibility.
Acta Physica Sinica, Chinese Physical Society and Institute of Physics, Chinese Academy of Sciences
Title: Multiple scattering and attenuation for electromagnetic wave propagation in sand and dust atmosphere
Description:
For an electronic system operation under the conditions of all-weather in arid and semiarid areas, the studies of the attenuation and multiple scattering are necessary for electromagnetic wave propagations in sand and dust atmosphere.
Based on Mie theory, a method of calculating the attenuations for electromagnetic wave propagation through sand and dust atmosphere is presented in this paper, which relate to the particle size distributions and visibilities for sand and dust atmosphere.
The attenuations at 37 GHz are given for various visibilities, and are compared with the results calculated from other formulas and the experimental data from the literature.
The attenuations are closer to the experimental results.
In order to investigate into electromagnetic wave propagations in lower visibility sand and dust atmosphere, the multiple scattering in sand and dust storms are necessarily analyzed.
At 37 and 93 GHz, the extinction cross sections, albedos and asymmetry factors are calculated by Mie theory for various size sand and dust particles.
By the Monte Carlo (MC) simulation method, the attenuations for including the multiple scattering effects are calculated under the conditions of dry and 5% water content in sand and dust particles, respectively, and are compared with the results from Mie theory.
The results are shown that the difference between the attenuation obtained by Mie and that by MC is small at 37 GHz.
The influence of the multiple scattering on attenuation is small and may be ignored at 37 GHz.
At 93 GHz, the difference between the attenuation obtained by Mie and that by MC is clear, and the attenuation obtained by using Mc simulation is smaller than that based on Mie theory.
The effect of the multiple scattering on attenuation is evident at 93 GHz.
The lower the visibility, the more notable the effect on attenuation is.
For different sand and dust storms, the particle refractive indexes and the particle size distributions are different.
For the sand and dust storms in Tengger desert and the blowing sand and dust atmosphere in north China, the attenuations at 93 GHz are analysed.
In Tengger desert, the attenuation and the multiple scattering are larger than in blowing sand and dust atmosphere.
The results show that the more the large size particles in sand and dust storms, the stronger the effect multiple scattering on attenuation is.
Hence, for stronger sand and dust storms, the attenuation and the effect of multiple scattering become important.
With the increase of water content in particle, the imaginary part of refractive index increases, the attenuation greatly increases, and the effect of the multiple scattering on attenuation is weakly varied.
The analyses show that the attenuations for electromagnetic wave propagation in arid sand and dust atmosphere are smaller than in moisture sand and dust atmosphere under the condition of the same visibility.

Related Results

Sand Production Management
Sand Production Management
Abstract Sand production may be inevitable in many fields that have a relatively lower formation strength. Sand erosion and settling predictions and sand monitori...
Linear polarization as a tool to characterize interplanetary, cometary, and extrasolar dust particles
Linear polarization as a tool to characterize interplanetary, cometary, and extrasolar dust particles
SummaryLinear polarization observations have suggested the presence of dust particles that scatter solar light within cometary comae and the interplanetary dust cloud. Recent progr...
Influence of sand and dust turbulent atmosphere on performance of free space quantum communication
Influence of sand and dust turbulent atmosphere on performance of free space quantum communication
Quantum communication is a frontier hotspot of current research, and it has ideal information security. In order to enable quantum systems in arid and desertified areas to work al...
Multi-Wave Joint Characterization Technique of Channel Sand Body in Shaximiao Formation, Northwestern Sichuan Basin
Multi-Wave Joint Characterization Technique of Channel Sand Body in Shaximiao Formation, Northwestern Sichuan Basin
Abstract The channel sand bodies in the first member of Middle Jurassic Shaximiao Formation (Sha 1 Member) in the northwest Sichuan basin ZT area shows a vertically ...
Modelling trajectories of wind-blown particles in the Martian atmosphere
Modelling trajectories of wind-blown particles in the Martian atmosphere
AbstractMartian dust storms can obscure the lower reaches of the atmosphere from orbiting spacecraft and at the same time obscure the upper atmosphere from landed spacecraft. Infer...
Dust deposition and lifting at the Zhurong landing site
Dust deposition and lifting at the Zhurong landing site
IntroductionDust deposition poses the challenges to the survival of instruments and solar-powered missions on Mars [1, 2]. Zhurong in-situ observations provide an opportunity to st...
The polarimetric dust properties of the debris disc HR479
The polarimetric dust properties of the debris disc HR479
ContextDebris discs represent the ultimate stage of planetary formation, after the initial gas-rich protoplanetary disc dissipated and potential giant planets have already formed i...

Back to Top