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Bernhardt PA, Hua M, Bortnik J, Ma Q, Verronen PT, McCarthy MP, Hampton DL, Golkowski M, Cohen MB, Richardson DK, Howarth AD, James HG, Meredith NP. Active Precipitation of Radiation Belt Electrons Using Rocket Exhaust Driven Amplification (REDA) of Man-Made Whistlers. JOURNAL OF GEOPHYSICAL RESEARCH. SPACE PHYSICS 2022; 127:e2022JA030358. [PMID: 35860435 PMCID: PMC9285445 DOI: 10.1029/2022ja030358] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Figures] [Subscribe] [Scholar Register] [Received: 02/07/2022] [Revised: 04/27/2022] [Accepted: 05/16/2022] [Indexed: 06/15/2023]
Abstract
Ground-based very low frequency (VLF) transmitters located around the world generate signals that leak through the bottom side of the ionosphere in the form of whistler mode waves. Wave and particle measurements on satellites have observed that these man-made VLF waves can be strong enough to scatter trapped energetic electrons into low pitch angle orbits, causing loss by absorption in the lower atmosphere. This precipitation loss process is greatly enhanced by intentional amplification of the whistler waves using a newly discovered process called rocket exhaust driven amplification (REDA). Satellite measurements of REDA have shown between 30 and 50 dB intensification of VLF waves in space using a 60 s burn of the 150 g/s thruster on the Cygnus satellite that services the International Space Station. This controlled amplification process is adequate to deplete the energetic particle population on the affected field lines in a few minutes rather than the multi-day period it would take naturally. Numerical simulations of the pitch angle diffusion for radiation belt particles use the UCLA quasi-linear Fokker Planck model to assess the impact of REDA on radiation belt remediation of newly injected energetic electrons. The simulated precipitation fluxes of energetic electrons are applied to models of D-region electron density and bremsstrahlung X-rays for predictions of the modified environment that can be observed with satellite and ground-based sensors.
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Affiliation(s)
| | - M. Hua
- Department of Atmospheric and Oceanography ScienceUCLALos AngelesCAUSA
| | - J. Bortnik
- Department of Atmospheric and Oceanography ScienceUCLALos AngelesCAUSA
| | - Q. Ma
- Department of Atmospheric and Oceanography ScienceUCLALos AngelesCAUSA
- Center for Space PhysicsBoston UniversityBostonMAUSA
| | - P. T. Verronen
- Sodankylä Geophysical ObservatoryUniversity of OuluSodankyläFinland
- Space and Earth Observation CentreFinnish Meteorological InstituteHelsinkiFinland
| | - M. P. McCarthy
- Department of Earth and Space SciencesUniversity of WashingtonSeattleWAUSA
| | - D. L. Hampton
- Geophysical InstituteUniversity of AlaskaFairbanksAKUSA
| | - M. Golkowski
- Department of Electrical EngineeringUniversity of Colorado DenverDenverCOUSA
| | - M. B. Cohen
- School of Electrical and Computer EngineeringGeorgia Institute of TechnologyAtlantaGAUSA
| | - D. K. Richardson
- School of Electrical and Computer EngineeringGeorgia Institute of TechnologyAtlantaGAUSA
| | - A. D. Howarth
- Department of Physics and AstronomyUniversity of CalgaryCalgaryABCanada
| | - H. G. James
- Department of Physics and AstronomyUniversity of CalgaryCalgaryABCanada
| | - N. P. Meredith
- British Antarctic SurveyNatural Environment Research CouncilCambridgeUK
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Khorashadizadeh SM, Abbasi S, Niknam AR, Vasheghani Farahani S, Fallah R. Rotating ion beam effects on temperature gradient instability in completely ionized plasmas. Phys Rev E 2020; 102:043208. [PMID: 33212659 DOI: 10.1103/physreve.102.043208] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 06/07/2020] [Accepted: 09/22/2020] [Indexed: 11/07/2022]
Abstract
The aim of this paper is to investigate the effects of a rotating ion beam on the temperature gradient instability (TGI) in completely ionized plasmas. The interplay of the temperature and density gradients provides the basis for experiencing an unstable inhomogeneous plasma medium due to TGI taken under consideration. The density and temperature gradients are considered perpendicular to the magnetic field where a nonrelativistic rotating ion beam such as O^{+} is present. By implementing the kinetic theory together with a zeroth-order approximation of geometrical optics, the dielectric permittivity tensor of the inhomogeneous plasma is obtained where by a suitable linear eikonal equation, the growth rate of the TGI in the collisional regime is calculated in the presence of a rotating ion beam. In such a configuration an unstable condition is experienced in regions with opposite electron density and temperature gradients, where it is destabilized by the temperature and plasma density gradients and the frequent electron collisions. As a consequence, the results reveal that the TGI can be damped or modified through interaction with the rotating ion beam depending on the characteristics of the ion beam, namely, velocity and density.
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Affiliation(s)
| | - S Abbasi
- Physics Department, University of Birjand, Birjand 97174 34765, Iran
| | - A R Niknam
- Laser and Plasma Research Institute, Shahid Beheshti University, Tehran 19839 69411, Iran
| | | | - R Fallah
- Physics Department, University of Birjand, Birjand 97174 34765, Iran
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Liu Y, Zhang Z, Lei J, Cao J, Yu P, Zhang X, Xu L, Zhao Y. Design and construction of Keda Space Plasma Experiment (KSPEX) for the investigation of the boundary layer processes of ionospheric depletions. THE REVIEW OF SCIENTIFIC INSTRUMENTS 2016; 87:093504. [PMID: 27782598 DOI: 10.1063/1.4962406] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/06/2023]
Abstract
In this work, the design and construction of the Keda Space Plasma EXperiment (KSPEX), which aims to study the boundary layer processes of ionospheric depletions, are described in detail. The device is composed of three stainless-steel sections: two source chambers at both ends and an experimental chamber in the center. KSPEX is a steady state experimental device, in which hot filament arrays are used to produce plasmas in the two sources. A Macor-mesh design is adopted to adjust the plasma density and potential difference between the two plasmas, which creates a boundary layer with a controllable electron density gradient and inhomogeneous radial electric field. In addition, attachment chemicals can be released into the plasmas through a tailor-made needle valve which leads to the generation of negative ions plasmas. Ionospheric depletions can be modeled and simulated using KSPEX, and many micro-physical processes of the formation and evolution of an ionospheric depletion can be experimentally studied.
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Affiliation(s)
- Yu Liu
- CAS Key Laboratory of Geospace Environment, School of Earth and Space Science, University of Science and Technology of China, Hefei 230026, China
| | - Zhongkai Zhang
- CAS Key Laboratory of Geospace Environment, Modern Physics Department, University of Science and Technology of China, Hefei 230026, China
| | - Jiuhou Lei
- CAS Key Laboratory of Geospace Environment, School of Earth and Space Science, University of Science and Technology of China, Hefei 230026, China
| | - Jinxiang Cao
- CAS Key Laboratory of Geospace Environment, Modern Physics Department, University of Science and Technology of China, Hefei 230026, China
| | - Pengcheng Yu
- CAS Key Laboratory of Geospace Environment, Modern Physics Department, University of Science and Technology of China, Hefei 230026, China
| | - Xiao Zhang
- CAS Key Laboratory of Geospace Environment, Modern Physics Department, University of Science and Technology of China, Hefei 230026, China
| | - Liang Xu
- CAS Key Laboratory of Geospace Environment, Modern Physics Department, University of Science and Technology of China, Hefei 230026, China
| | - Yaodong Zhao
- CAS Key Laboratory of Geospace Environment, Modern Physics Department, University of Science and Technology of China, Hefei 230026, China
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Ganguli G, Rudakov L, Mithaiwala M, Papadopoulos K. Generation and evolution of intense ion cyclotron turbulence by artificial plasma cloud in the magnetosphere. ACTA ACUST UNITED AC 2007. [DOI: 10.1029/2006ja012162] [Citation(s) in RCA: 15] [Impact Index Per Article: 0.9] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
Affiliation(s)
- Gurudas Ganguli
- Plasma Physics Division; Naval Research Laboratory; Washington District of Columbia USA
| | | | - Manish Mithaiwala
- National Research Council, Naval Research Laboratory; Washington District of Columbia USA
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