Radiation-Belt Remediation Using Space-Based Antennas and Electron Beams
Energetic electrons can be trapped in Earth's magnetic field, forming the radiation belts (also known as the Van Allen Belts). These electrons, which can originate from the solar wind or a high-altitude nuclear explosion (HANE), have the potential to damage satellites in low-Earth orbit (LEO)....
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Veröffentlicht in: | IEEE transactions on plasma science 2019-05, Vol.47 (5), p.2045-2063 |
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creator | Carlsten, Bruce E. Colestock, Patrick L. Cunningham, Gregory S. Delzanno, Gian Luca Dors, Eric E. Holloway, Michael A. Jeffery, Christopher A. Lewellen, John W. Marksteiner, Quinn R. Nguyen, Dinh C. Reeves, Geoffrey D. Shipman, Kevin A. |
description | Energetic electrons can be trapped in Earth's magnetic field, forming the radiation belts (also known as the Van Allen Belts). These electrons, which can originate from the solar wind or a high-altitude nuclear explosion (HANE), have the potential to damage satellites in low-Earth orbit (LEO). For example, in 1962, the U.S. detonated a nuclear device at an altitude of about 400 km in the Starfish experiment. The resulting enhancement of the radiation belts disabled several satellites within a few months and energetic electrons remained in the radiation belts for up to several years. In order to address this potential vulnerability, schemes have been proposed to drain electrons from the radiation belts, with the most promising approaches based on using high-power very-low-frequency (VLF) waves to scatter the electrons into more field-aligned trajectories, forcing them to precipitate into Earth's atmosphere. This paper will provide an overview of enhanced electron distributions in the radiation belts as well as approaches to VLF wave belt remediation including the use of either antennas or relativistic electrons beams in space to generate the VLF waves. |
doi_str_mv | 10.1109/TPS.2019.2910829 |
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These electrons, which can originate from the solar wind or a high-altitude nuclear explosion (HANE), have the potential to damage satellites in low-Earth orbit (LEO). For example, in 1962, the U.S. detonated a nuclear device at an altitude of about 400 km in the Starfish experiment. The resulting enhancement of the radiation belts disabled several satellites within a few months and energetic electrons remained in the radiation belts for up to several years. In order to address this potential vulnerability, schemes have been proposed to drain electrons from the radiation belts, with the most promising approaches based on using high-power very-low-frequency (VLF) waves to scatter the electrons into more field-aligned trajectories, forcing them to precipitate into Earth's atmosphere. This paper will provide an overview of enhanced electron distributions in the radiation belts as well as approaches to VLF wave belt remediation including the use of either antennas or relativistic electrons beams in space to generate the VLF waves.</description><identifier>ISSN: 0093-3813</identifier><identifier>EISSN: 1939-9375</identifier><identifier>DOI: 10.1109/TPS.2019.2910829</identifier><identifier>CODEN: ITPSBD</identifier><language>eng</language><publisher>New York: IEEE</publisher><subject>Accelerators ; Antennas ; Detonation ; Earth ; Earth orbits ; Electron beams ; Electron traps ; Electrons ; High altitude ; Ionizing radiation ; ionosphere ; Jupiter ; Low earth orbits ; Magnetic fields ; Mirrors ; Radiation ; Radiation belts ; Remediation ; Satellites ; Solar radiation ; Solar wind ; Space radiation ; Space vehicles ; Very Low Frequencies</subject><ispartof>IEEE transactions on plasma science, 2019-05, Vol.47 (5), p.2045-2063</ispartof><rights>Copyright The Institute of Electrical and Electronics Engineers, Inc. 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These electrons, which can originate from the solar wind or a high-altitude nuclear explosion (HANE), have the potential to damage satellites in low-Earth orbit (LEO). For example, in 1962, the U.S. detonated a nuclear device at an altitude of about 400 km in the Starfish experiment. The resulting enhancement of the radiation belts disabled several satellites within a few months and energetic electrons remained in the radiation belts for up to several years. In order to address this potential vulnerability, schemes have been proposed to drain electrons from the radiation belts, with the most promising approaches based on using high-power very-low-frequency (VLF) waves to scatter the electrons into more field-aligned trajectories, forcing them to precipitate into Earth's atmosphere. This paper will provide an overview of enhanced electron distributions in the radiation belts as well as approaches to VLF wave belt remediation including the use of either antennas or relativistic electrons beams in space to generate the VLF waves.</description><subject>Accelerators</subject><subject>Antennas</subject><subject>Detonation</subject><subject>Earth</subject><subject>Earth orbits</subject><subject>Electron beams</subject><subject>Electron traps</subject><subject>Electrons</subject><subject>High altitude</subject><subject>Ionizing radiation</subject><subject>ionosphere</subject><subject>Jupiter</subject><subject>Low earth orbits</subject><subject>Magnetic fields</subject><subject>Mirrors</subject><subject>Radiation</subject><subject>Radiation belts</subject><subject>Remediation</subject><subject>Satellites</subject><subject>Solar radiation</subject><subject>Solar wind</subject><subject>Space radiation</subject><subject>Space vehicles</subject><subject>Very Low Frequencies</subject><issn>0093-3813</issn><issn>1939-9375</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2019</creationdate><recordtype>article</recordtype><sourceid>RIE</sourceid><recordid>eNo9kE1LAzEQhoMoWKt3wcuC560zSfcjx7aoFQpKP84hHxPZ0mZrsj34793S4lxeGJ53Bh7GHhFGiCBf1l-rEQeUIy4Rai6v2AClkLkUVXHNBgBS5KJGccvuUtoC4LgAPmDzpXaN7po25FPaddmS9nRZZJvUhO9sddCW8qlO5LJJ6CgEnTIdXPa6I9vFnpuS3qd7duP1LtHDJYds8_a6ns3zxef7x2yyyK0QdZdXzmAJjpdaE5bCeWfImxqNozF3prRQGYGmrATWhbfgKu9LMl5bLfsWiSF7Pt89xPbnSKlT2_YYQ_9S8X5QSllAT8GZsrFNKZJXh9jsdfxVCOrkS_W-1MmXuvjqK0_nSkNE_3hdgZTIxR_pM2cg</recordid><startdate>20190501</startdate><enddate>20190501</enddate><creator>Carlsten, Bruce E.</creator><creator>Colestock, Patrick L.</creator><creator>Cunningham, Gregory S.</creator><creator>Delzanno, Gian Luca</creator><creator>Dors, Eric E.</creator><creator>Holloway, Michael A.</creator><creator>Jeffery, Christopher A.</creator><creator>Lewellen, John W.</creator><creator>Marksteiner, Quinn R.</creator><creator>Nguyen, Dinh C.</creator><creator>Reeves, Geoffrey D.</creator><creator>Shipman, Kevin A.</creator><general>IEEE</general><general>The Institute of Electrical and Electronics Engineers, Inc. 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These electrons, which can originate from the solar wind or a high-altitude nuclear explosion (HANE), have the potential to damage satellites in low-Earth orbit (LEO). For example, in 1962, the U.S. detonated a nuclear device at an altitude of about 400 km in the Starfish experiment. The resulting enhancement of the radiation belts disabled several satellites within a few months and energetic electrons remained in the radiation belts for up to several years. In order to address this potential vulnerability, schemes have been proposed to drain electrons from the radiation belts, with the most promising approaches based on using high-power very-low-frequency (VLF) waves to scatter the electrons into more field-aligned trajectories, forcing them to precipitate into Earth's atmosphere. 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subjects | Accelerators Antennas Detonation Earth Earth orbits Electron beams Electron traps Electrons High altitude Ionizing radiation ionosphere Jupiter Low earth orbits Magnetic fields Mirrors Radiation Radiation belts Remediation Satellites Solar radiation Solar wind Space radiation Space vehicles Very Low Frequencies |
title | Radiation-Belt Remediation Using Space-Based Antennas and Electron Beams |
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