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Modeling the relativistic runaway electron avalanche and the feedback mechanism with GEANT4
This paper presents the first study that uses the GEometry ANd Tracking 4 (GEANT4) toolkit to do quantitative comparisons with other modeling results related to the production of terrestrial gamma ray flashes and high‐energy particle emission from thunderstorms. We will study the relativistic runawa...
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Published in: | Journal of geophysical research. Space physics 2014-11, Vol.119 (11), p.9174-9191 |
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creator | Skeltved, Alexander Broberg Østgaard, Nikolai Carlson, Brant Gjesteland, Thomas Celestin, Sebastien |
description | This paper presents the first study that uses the GEometry ANd Tracking 4 (GEANT4) toolkit to do quantitative comparisons with other modeling results related to the production of terrestrial gamma ray flashes and high‐energy particle emission from thunderstorms. We will study the relativistic runaway electron avalanche (RREA) and the relativistic feedback process, as well as the production of bremsstrahlung photons from runaway electrons. The Monte Carlo simulations take into account the effects of electron ionization, electron by electron (Møller), and electron by positron (Bhabha) scattering as well as the bremsstrahlung process and pair production, in the 250 eV to 100 GeV energy range. Our results indicate that the multiplication of electrons during the development of RREAs and under the influence of feedback are consistent with previous estimates. This is important to validate GEANT4 as a tool to model RREAs and feedback in homogeneous electric fields. We also determine the ratio of bremsstrahlung photons to energetic electrons Nγ/Ne. We then show that the ratio has a dependence on the electric field, which can be expressed by the avalanche time τ(E) and the bremsstrahlung coefficient α(ϵ). In addition, we present comparisons of GEANT4 simulations performed with a “standard” and a “low‐energy” physics list both validated in the 1 keV to 100 GeV energy range. This comparison shows that the choice of physics list used in GEANT4 simulations has a significant effect on the results.
Key Points
Testing the feedback mechanism with GEANT4Validating the GEANT4 programming toolkitStudy the ratio of bremsstrahlung photons to electrons at TGF source altitude |
doi_str_mv | 10.1002/2014JA020504 |
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Key Points
Testing the feedback mechanism with GEANT4Validating the GEANT4 programming toolkitStudy the ratio of bremsstrahlung photons to electrons at TGF source altitude</description><identifier>ISSN: 2169-9380</identifier><identifier>EISSN: 2169-9402</identifier><identifier>DOI: 10.1002/2014JA020504</identifier><identifier>PMID: 26167437</identifier><language>eng</language><publisher>United States: Blackwell Publishing Ltd</publisher><subject>Bremsstrahlung ; Computer simulation ; Electric fields ; Electron avalanche ; Energy ; Feedback ; Gamma rays ; Ionization ; lightning ; Lists ; Monte Carlo simulation ; Photons ; Physics ; Relativism ; RREA ; runaway relativistic electron avalanche ; Sciences of the Universe ; terrestrial gamma ray flashes ; TGF ; Thunderstorms</subject><ispartof>Journal of geophysical research. Space physics, 2014-11, Vol.119 (11), p.9174-9191</ispartof><rights>2014. The Authors.</rights><rights>2014. American Geophysical Union. All Rights Reserved.</rights><rights>Distributed under a Creative Commons Attribution 4.0 International License</rights><rights>2014. The Authors. 2014</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c6650-ee6c9a3b393b8aa83120d4849874c68ea8fabd2bb3c83a4e69022f93626f2e643</citedby><cites>FETCH-LOGICAL-c6650-ee6c9a3b393b8aa83120d4849874c68ea8fabd2bb3c83a4e69022f93626f2e643</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,314,780,784,885,27923,27924</link.rule.ids><backlink>$$Uhttps://www.ncbi.nlm.nih.gov/pubmed/26167437$$D View this record in MEDLINE/PubMed$$Hfree_for_read</backlink><backlink>$$Uhttps://insu.hal.science/insu-01259449$$DView record in HAL$$Hfree_for_read</backlink></links><search><creatorcontrib>Skeltved, Alexander Broberg</creatorcontrib><creatorcontrib>Østgaard, Nikolai</creatorcontrib><creatorcontrib>Carlson, Brant</creatorcontrib><creatorcontrib>Gjesteland, Thomas</creatorcontrib><creatorcontrib>Celestin, Sebastien</creatorcontrib><title>Modeling the relativistic runaway electron avalanche and the feedback mechanism with GEANT4</title><title>Journal of geophysical research. Space physics</title><addtitle>J. Geophys. Res. Space Physics</addtitle><description>This paper presents the first study that uses the GEometry ANd Tracking 4 (GEANT4) toolkit to do quantitative comparisons with other modeling results related to the production of terrestrial gamma ray flashes and high‐energy particle emission from thunderstorms. We will study the relativistic runaway electron avalanche (RREA) and the relativistic feedback process, as well as the production of bremsstrahlung photons from runaway electrons. The Monte Carlo simulations take into account the effects of electron ionization, electron by electron (Møller), and electron by positron (Bhabha) scattering as well as the bremsstrahlung process and pair production, in the 250 eV to 100 GeV energy range. Our results indicate that the multiplication of electrons during the development of RREAs and under the influence of feedback are consistent with previous estimates. This is important to validate GEANT4 as a tool to model RREAs and feedback in homogeneous electric fields. We also determine the ratio of bremsstrahlung photons to energetic electrons Nγ/Ne. We then show that the ratio has a dependence on the electric field, which can be expressed by the avalanche time τ(E) and the bremsstrahlung coefficient α(ϵ). In addition, we present comparisons of GEANT4 simulations performed with a “standard” and a “low‐energy” physics list both validated in the 1 keV to 100 GeV energy range. This comparison shows that the choice of physics list used in GEANT4 simulations has a significant effect on the results.
Key Points
Testing the feedback mechanism with GEANT4Validating the GEANT4 programming toolkitStudy the ratio of bremsstrahlung photons to electrons at TGF source altitude</description><subject>Bremsstrahlung</subject><subject>Computer simulation</subject><subject>Electric fields</subject><subject>Electron avalanche</subject><subject>Energy</subject><subject>Feedback</subject><subject>Gamma rays</subject><subject>Ionization</subject><subject>lightning</subject><subject>Lists</subject><subject>Monte Carlo simulation</subject><subject>Photons</subject><subject>Physics</subject><subject>Relativism</subject><subject>RREA</subject><subject>runaway relativistic electron avalanche</subject><subject>Sciences of the Universe</subject><subject>terrestrial gamma ray flashes</subject><subject>TGF</subject><subject>Thunderstorms</subject><issn>2169-9380</issn><issn>2169-9402</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2014</creationdate><recordtype>article</recordtype><sourceid>24P</sourceid><recordid>eNqNkttrFDEYxQdRbKl981kGfBFxNffLi7AsdWtZq5RKBR9CJvNNJ-1cajKz2_3vm7rtUvug5iUh-Z0TvsPJspcYvccIkQ8EYXY0RQRxxJ5kuwQLPdEMkaf3Z6rQTrYf4wVKS6UrzJ9nO0RgIRmVu9nPL30Jje_O86GGPEBjB7_0cfAuD2NnV3adQwNuCH2X26VtbOcSZ7vyN18BlIV1l3kLrradj22-8kOdzw-mx6fsRfassk2E_bt9L_v-6eB0djhZfJ1_nk0XEycERxMA4bSlBdW0UNYqigkqmWJaSeaEAqsqW5SkKKhT1DIQGhFSaSqIqAgIRveyjxvfq7FooXTQDcE25ir41oa16a03f750vjbn_dIwpiXjOhm83RjUj2SH04XxXRwNwoTrhC9xgt_c_Rb6XyPEwbQ-OmhSNNCP0WBFhCBMM_VvVHDMGOZC_wfKJMJcyttxXz9CL_oxdCnhRFEtEeOCJOrdhnKhjzFAtR0MI3PbHfOwOwl_9TDDLXzflATQDbDyDaz_amaO5idTjqlGSTXZqFKl4HqrsuHSCEklN2fHcyNnP2ZnVH4zJ_QGgbTaHg</recordid><startdate>201411</startdate><enddate>201411</enddate><creator>Skeltved, Alexander Broberg</creator><creator>Østgaard, Nikolai</creator><creator>Carlson, Brant</creator><creator>Gjesteland, Thomas</creator><creator>Celestin, Sebastien</creator><general>Blackwell Publishing Ltd</general><general>American Geophysical Union/Wiley</general><scope>BSCLL</scope><scope>24P</scope><scope>WIN</scope><scope>NPM</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>8FD</scope><scope>H8D</scope><scope>KL.</scope><scope>L7M</scope><scope>7X8</scope><scope>1XC</scope><scope>VOOES</scope><scope>5PM</scope></search><sort><creationdate>201411</creationdate><title>Modeling the relativistic runaway electron avalanche and the feedback mechanism with GEANT4</title><author>Skeltved, Alexander Broberg ; Østgaard, Nikolai ; Carlson, Brant ; Gjesteland, Thomas ; Celestin, Sebastien</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c6650-ee6c9a3b393b8aa83120d4849874c68ea8fabd2bb3c83a4e69022f93626f2e643</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2014</creationdate><topic>Bremsstrahlung</topic><topic>Computer simulation</topic><topic>Electric fields</topic><topic>Electron avalanche</topic><topic>Energy</topic><topic>Feedback</topic><topic>Gamma rays</topic><topic>Ionization</topic><topic>lightning</topic><topic>Lists</topic><topic>Monte Carlo simulation</topic><topic>Photons</topic><topic>Physics</topic><topic>Relativism</topic><topic>RREA</topic><topic>runaway relativistic electron avalanche</topic><topic>Sciences of the Universe</topic><topic>terrestrial gamma ray flashes</topic><topic>TGF</topic><topic>Thunderstorms</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Skeltved, Alexander Broberg</creatorcontrib><creatorcontrib>Østgaard, Nikolai</creatorcontrib><creatorcontrib>Carlson, Brant</creatorcontrib><creatorcontrib>Gjesteland, Thomas</creatorcontrib><creatorcontrib>Celestin, Sebastien</creatorcontrib><collection>Istex</collection><collection>Open Access: Wiley-Blackwell Open Access Journals</collection><collection>Wiley Online Library Journals</collection><collection>PubMed</collection><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>MEDLINE - Academic</collection><collection>Hyper Article en Ligne (HAL)</collection><collection>Hyper Article en Ligne (HAL) (Open Access)</collection><collection>PubMed Central (Full Participant titles)</collection><jtitle>Journal of geophysical research. Space physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Skeltved, Alexander Broberg</au><au>Østgaard, Nikolai</au><au>Carlson, Brant</au><au>Gjesteland, Thomas</au><au>Celestin, Sebastien</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Modeling the relativistic runaway electron avalanche and the feedback mechanism with GEANT4</atitle><jtitle>Journal of geophysical research. Space physics</jtitle><addtitle>J. Geophys. Res. Space Physics</addtitle><date>2014-11</date><risdate>2014</risdate><volume>119</volume><issue>11</issue><spage>9174</spage><epage>9191</epage><pages>9174-9191</pages><issn>2169-9380</issn><eissn>2169-9402</eissn><abstract>This paper presents the first study that uses the GEometry ANd Tracking 4 (GEANT4) toolkit to do quantitative comparisons with other modeling results related to the production of terrestrial gamma ray flashes and high‐energy particle emission from thunderstorms. We will study the relativistic runaway electron avalanche (RREA) and the relativistic feedback process, as well as the production of bremsstrahlung photons from runaway electrons. The Monte Carlo simulations take into account the effects of electron ionization, electron by electron (Møller), and electron by positron (Bhabha) scattering as well as the bremsstrahlung process and pair production, in the 250 eV to 100 GeV energy range. Our results indicate that the multiplication of electrons during the development of RREAs and under the influence of feedback are consistent with previous estimates. This is important to validate GEANT4 as a tool to model RREAs and feedback in homogeneous electric fields. We also determine the ratio of bremsstrahlung photons to energetic electrons Nγ/Ne. We then show that the ratio has a dependence on the electric field, which can be expressed by the avalanche time τ(E) and the bremsstrahlung coefficient α(ϵ). In addition, we present comparisons of GEANT4 simulations performed with a “standard” and a “low‐energy” physics list both validated in the 1 keV to 100 GeV energy range. This comparison shows that the choice of physics list used in GEANT4 simulations has a significant effect on the results.
Key Points
Testing the feedback mechanism with GEANT4Validating the GEANT4 programming toolkitStudy the ratio of bremsstrahlung photons to electrons at TGF source altitude</abstract><cop>United States</cop><pub>Blackwell Publishing Ltd</pub><pmid>26167437</pmid><doi>10.1002/2014JA020504</doi><tpages>18</tpages><oa>free_for_read</oa></addata></record> |
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subjects | Bremsstrahlung Computer simulation Electric fields Electron avalanche Energy Feedback Gamma rays Ionization lightning Lists Monte Carlo simulation Photons Physics Relativism RREA runaway relativistic electron avalanche Sciences of the Universe terrestrial gamma ray flashes TGF Thunderstorms |
title | Modeling the relativistic runaway electron avalanche and the feedback mechanism with GEANT4 |
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