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Properties of relatively long streamers initiated from an isolated hydrometeor

This paper reports a modeling study on the dynamics of relatively long streamers initiated from an isolated hydrometeor in subbreakdown (0.5Ek) and overbreakdown (1.5Ek) electric fields, respectively, where Ek is the conventional breakdown threshold field. The modeling results indicate that at 0.5Ek...

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Published in:Journal of geophysical research. Atmospheres 2016-06, Vol.121 (12), p.7284-7295
Main Authors: Shi, Feng, Liu, Ningyu, Rassoul, Hamid K.
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Liu, Ningyu
Rassoul, Hamid K.
description This paper reports a modeling study on the dynamics of relatively long streamers initiated from an isolated hydrometeor in subbreakdown (0.5Ek) and overbreakdown (1.5Ek) electric fields, respectively, where Ek is the conventional breakdown threshold field. The modeling results indicate that at 0.5Ek field, the streamer shows a generally exponential growth feature, but its channel characteristics such as radius, electron density, and current density exhibit colocated fluctuations. On the other hand, at 1.5Ek field, the streamer shows faster exponential growth, and no fluctuations of those parameters are observed. The exponential growth property allows one to use the modeling results to predict the characteristics of longer streamers, as well as to quantify the thunderstorm electrical conditions including the high‐field region size and potential difference in order to accelerate the streamer to the high speed of fast positive breakdown that was observed recently in lightning initiation. At 0.5Ek, a potential difference of ∼0.3–1.8 MV is required to accelerate the streamer to the high speed of 1–5 × 107 m/s, while at 1.5Ek, ∼0.07–0.4 MV is required. The exponentially growing streamer current produces an exponentially increasing magnetic field, leading to electromagnetic (EM) field radiation. It is found that the growth rate of the magnetic field ( 1/τBϕ) radiated by a streamer can be obtained by a simple relation 1/τBϕ∼3/τ, where 1/τ is the growth rate of the streamer. Combining our modeling results with the Fourier analysis reported by Qin et al. (2012), we find that streamers at thundercloud altitudes radiate in the high frequency and very high frequency range of the EM spectrum. Key Points Thunderstorm streamers grow exponentially, but the exponential growth may display fluctuation The exponentially growing streamers emit HF and VHF EM radiation A thundercloud potential difference of 0.1–1 MV is required to accelerate streamers to 10,000 km/s
doi_str_mv 10.1002/2015JD024580
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The modeling results indicate that at 0.5Ek field, the streamer shows a generally exponential growth feature, but its channel characteristics such as radius, electron density, and current density exhibit colocated fluctuations. On the other hand, at 1.5Ek field, the streamer shows faster exponential growth, and no fluctuations of those parameters are observed. The exponential growth property allows one to use the modeling results to predict the characteristics of longer streamers, as well as to quantify the thunderstorm electrical conditions including the high‐field region size and potential difference in order to accelerate the streamer to the high speed of fast positive breakdown that was observed recently in lightning initiation. At 0.5Ek, a potential difference of ∼0.3–1.8 MV is required to accelerate the streamer to the high speed of 1–5 × 107 m/s, while at 1.5Ek, ∼0.07–0.4 MV is required. The exponentially growing streamer current produces an exponentially increasing magnetic field, leading to electromagnetic (EM) field radiation. It is found that the growth rate of the magnetic field ( 1/τBϕ) radiated by a streamer can be obtained by a simple relation 1/τBϕ∼3/τ, where 1/τ is the growth rate of the streamer. Combining our modeling results with the Fourier analysis reported by Qin et al. (2012), we find that streamers at thundercloud altitudes radiate in the high frequency and very high frequency range of the EM spectrum. Key Points Thunderstorm streamers grow exponentially, but the exponential growth may display fluctuation The exponentially growing streamers emit HF and VHF EM radiation A thundercloud potential difference of 0.1–1 MV is required to accelerate streamers to 10,000 km/s</description><identifier>ISSN: 2169-897X</identifier><identifier>EISSN: 2169-8996</identifier><identifier>DOI: 10.1002/2015JD024580</identifier><language>eng</language><publisher>Washington: Blackwell Publishing Ltd</publisher><subject>Breakdown ; Current density ; Dynamics ; Electric field ; Electric fields ; Electric potential ; Electromagnetic radiation ; Electron density ; Fields ; Fluctuation ; Fluctuations ; Fourier analysis ; Geophysics ; Growth rate ; High frequency ; High speed ; Hydrometeors ; Lightning ; long streamer ; Magnetic field ; Magnetic fields ; Mathematical models ; Modelling ; Parameters ; Properties ; Radiation ; streamer propagation ; streamer radiation ; Streamers ; Thunderstorms ; Very high frequencies</subject><ispartof>Journal of geophysical research. 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Atmospheres</title><description>This paper reports a modeling study on the dynamics of relatively long streamers initiated from an isolated hydrometeor in subbreakdown (0.5Ek) and overbreakdown (1.5Ek) electric fields, respectively, where Ek is the conventional breakdown threshold field. The modeling results indicate that at 0.5Ek field, the streamer shows a generally exponential growth feature, but its channel characteristics such as radius, electron density, and current density exhibit colocated fluctuations. On the other hand, at 1.5Ek field, the streamer shows faster exponential growth, and no fluctuations of those parameters are observed. The exponential growth property allows one to use the modeling results to predict the characteristics of longer streamers, as well as to quantify the thunderstorm electrical conditions including the high‐field region size and potential difference in order to accelerate the streamer to the high speed of fast positive breakdown that was observed recently in lightning initiation. At 0.5Ek, a potential difference of ∼0.3–1.8 MV is required to accelerate the streamer to the high speed of 1–5 × 107 m/s, while at 1.5Ek, ∼0.07–0.4 MV is required. The exponentially growing streamer current produces an exponentially increasing magnetic field, leading to electromagnetic (EM) field radiation. It is found that the growth rate of the magnetic field ( 1/τBϕ) radiated by a streamer can be obtained by a simple relation 1/τBϕ∼3/τ, where 1/τ is the growth rate of the streamer. Combining our modeling results with the Fourier analysis reported by Qin et al. (2012), we find that streamers at thundercloud altitudes radiate in the high frequency and very high frequency range of the EM spectrum. 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Atmospheres</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Shi, Feng</au><au>Liu, Ningyu</au><au>Rassoul, Hamid K.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Properties of relatively long streamers initiated from an isolated hydrometeor</atitle><jtitle>Journal of geophysical research. Atmospheres</jtitle><date>2016-06-27</date><risdate>2016</risdate><volume>121</volume><issue>12</issue><spage>7284</spage><epage>7295</epage><pages>7284-7295</pages><issn>2169-897X</issn><eissn>2169-8996</eissn><abstract>This paper reports a modeling study on the dynamics of relatively long streamers initiated from an isolated hydrometeor in subbreakdown (0.5Ek) and overbreakdown (1.5Ek) electric fields, respectively, where Ek is the conventional breakdown threshold field. The modeling results indicate that at 0.5Ek field, the streamer shows a generally exponential growth feature, but its channel characteristics such as radius, electron density, and current density exhibit colocated fluctuations. On the other hand, at 1.5Ek field, the streamer shows faster exponential growth, and no fluctuations of those parameters are observed. The exponential growth property allows one to use the modeling results to predict the characteristics of longer streamers, as well as to quantify the thunderstorm electrical conditions including the high‐field region size and potential difference in order to accelerate the streamer to the high speed of fast positive breakdown that was observed recently in lightning initiation. At 0.5Ek, a potential difference of ∼0.3–1.8 MV is required to accelerate the streamer to the high speed of 1–5 × 107 m/s, while at 1.5Ek, ∼0.07–0.4 MV is required. The exponentially growing streamer current produces an exponentially increasing magnetic field, leading to electromagnetic (EM) field radiation. It is found that the growth rate of the magnetic field ( 1/τBϕ) radiated by a streamer can be obtained by a simple relation 1/τBϕ∼3/τ, where 1/τ is the growth rate of the streamer. Combining our modeling results with the Fourier analysis reported by Qin et al. (2012), we find that streamers at thundercloud altitudes radiate in the high frequency and very high frequency range of the EM spectrum. 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subjects Breakdown
Current density
Dynamics
Electric field
Electric fields
Electric potential
Electromagnetic radiation
Electron density
Fields
Fluctuation
Fluctuations
Fourier analysis
Geophysics
Growth rate
High frequency
High speed
Hydrometeors
Lightning
long streamer
Magnetic field
Magnetic fields
Mathematical models
Modelling
Parameters
Properties
Radiation
streamer propagation
streamer radiation
Streamers
Thunderstorms
Very high frequencies
title Properties of relatively long streamers initiated from an isolated hydrometeor
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