Toward An Integrated View of Ionospheric Plasma Instabilities: 5. Ion‐Thermal Instability for Arbitrary Ion Magnetization, Density Gradient, and Wave Propagation

A unified fluid theory of ionospheric electrostatic instabilities is presented that includes thermal effects due to nonisothermal processes for arbitrary ion magnetization, background density gradient, and wave propagation. The theory considers arbitrary altitude within the limits imposed by the flu...

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Veröffentlicht in:Journal of geophysical research. Space physics 2020-09, Vol.125 (9), p.n/a
1. Verfasser: Makarevich, Roman A.
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description A unified fluid theory of ionospheric electrostatic instabilities is presented that includes thermal effects due to nonisothermal processes for arbitrary ion magnetization, background density gradient, and wave propagation. The theory considers arbitrary altitude within the limits imposed by the fluid and collisional models and integrates the ion‐thermal instability (ITI) with the Farley‐Buneman and gradient‐drift plasma instabilities (FBI and GDI). A general dispersion relation is obtained and solved numerically for the complex wave frequency ω by using either an iterative or a polynomial (quadric) form in ω. An analytic explicit expression for the instability growth rate is also derived under the local and slow growth approximations. The previously considered limiting cases of the FBI/ITI at long wavelengths and the FBI/GDI for isothermal plasma are successfully recovered. In the high‐latitude E‐region near 110 km in altitude, thermal effects are found to be destabilizing at long wavelengths near λ=1,000 m and stabilizing at shorter wavelengths near 10 m. In the F‐region, the effects are destabilizing at λ=1,000 m but much weaker that those of GDI for moderate gradients. At shorter wavelengths, they become comparable so that a significant fraction of propagation directions at λ=10 m have positive growth rates, in contrast with the isothermal FBI/GDI case, where stronger gradients are needed to destabilize the plasma at these short wavelengths. The overall conclusion is that the thermal effects modify the growth rate terms traditionally associated with FBI and GDI rather than being purely additive. Key Points Unified theory is developed for the ion‐thermal, Farley‐Buneman, and gradient‐drift instabilities for any magnetization and gradient Thermal effects modify the Farley‐Buneman and gradient‐drift factors, while being modified by inertia, rather than being purely additive Thermal effects can help destabilize the plasma at long scales in the E‐region and at short scales in the F‐region
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Ion‐Thermal Instability for Arbitrary Ion Magnetization, Density Gradient, and Wave Propagation</title><source>Wiley-Blackwell Journals</source><source>Wiley Online Library Journals</source><creator>Makarevich, Roman A.</creator><creatorcontrib>Makarevich, Roman A.</creatorcontrib><description>A unified fluid theory of ionospheric electrostatic instabilities is presented that includes thermal effects due to nonisothermal processes for arbitrary ion magnetization, background density gradient, and wave propagation. The theory considers arbitrary altitude within the limits imposed by the fluid and collisional models and integrates the ion‐thermal instability (ITI) with the Farley‐Buneman and gradient‐drift plasma instabilities (FBI and GDI). A general dispersion relation is obtained and solved numerically for the complex wave frequency ω by using either an iterative or a polynomial (quadric) form in ω. An analytic explicit expression for the instability growth rate is also derived under the local and slow growth approximations. The previously considered limiting cases of the FBI/ITI at long wavelengths and the FBI/GDI for isothermal plasma are successfully recovered. In the high‐latitude E‐region near 110 km in altitude, thermal effects are found to be destabilizing at long wavelengths near λ=1,000 m and stabilizing at shorter wavelengths near 10 m. In the F‐region, the effects are destabilizing at λ=1,000 m but much weaker that those of GDI for moderate gradients. At shorter wavelengths, they become comparable so that a significant fraction of propagation directions at λ=10 m have positive growth rates, in contrast with the isothermal FBI/GDI case, where stronger gradients are needed to destabilize the plasma at these short wavelengths. The overall conclusion is that the thermal effects modify the growth rate terms traditionally associated with FBI and GDI rather than being purely additive. Key Points Unified theory is developed for the ion‐thermal, Farley‐Buneman, and gradient‐drift instabilities for any magnetization and gradient Thermal effects modify the Farley‐Buneman and gradient‐drift factors, while being modified by inertia, rather than being purely additive Thermal effects can help destabilize the plasma at long scales in the E‐region and at short scales in the F‐region</description><identifier>ISSN: 2169-9380</identifier><identifier>EISSN: 2169-9402</identifier><identifier>DOI: 10.1029/2020JA028349</identifier><language>eng</language><publisher>Washington: Blackwell Publishing Ltd</publisher><subject>Altitude ; Altitude effects ; Density ; Density gradients ; E region ; F region ; Instability ; Ion thermal instability ; Ionospheric plasma ; Ionospheric propagation ; Iterative methods ; Magnetization ; Magnetohydrodynamic stability ; Nonisothermal processes ; Plasma ; Plasma instabilities ; plasma instability ; Polynomials ; Propagation ; Stability analysis ; Temperature effects ; thermal effects ; Thermal instability ; Wave propagation ; Wavelengths</subject><ispartof>Journal of geophysical research. Space physics, 2020-09, Vol.125 (9), p.n/a</ispartof><rights>2020. American Geophysical Union. 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Ion‐Thermal Instability for Arbitrary Ion Magnetization, Density Gradient, and Wave Propagation</title><title>Journal of geophysical research. Space physics</title><description>A unified fluid theory of ionospheric electrostatic instabilities is presented that includes thermal effects due to nonisothermal processes for arbitrary ion magnetization, background density gradient, and wave propagation. The theory considers arbitrary altitude within the limits imposed by the fluid and collisional models and integrates the ion‐thermal instability (ITI) with the Farley‐Buneman and gradient‐drift plasma instabilities (FBI and GDI). A general dispersion relation is obtained and solved numerically for the complex wave frequency ω by using either an iterative or a polynomial (quadric) form in ω. An analytic explicit expression for the instability growth rate is also derived under the local and slow growth approximations. The previously considered limiting cases of the FBI/ITI at long wavelengths and the FBI/GDI for isothermal plasma are successfully recovered. In the high‐latitude E‐region near 110 km in altitude, thermal effects are found to be destabilizing at long wavelengths near λ=1,000 m and stabilizing at shorter wavelengths near 10 m. In the F‐region, the effects are destabilizing at λ=1,000 m but much weaker that those of GDI for moderate gradients. At shorter wavelengths, they become comparable so that a significant fraction of propagation directions at λ=10 m have positive growth rates, in contrast with the isothermal FBI/GDI case, where stronger gradients are needed to destabilize the plasma at these short wavelengths. The overall conclusion is that the thermal effects modify the growth rate terms traditionally associated with FBI and GDI rather than being purely additive. Key Points Unified theory is developed for the ion‐thermal, Farley‐Buneman, and gradient‐drift instabilities for any magnetization and gradient Thermal effects modify the Farley‐Buneman and gradient‐drift factors, while being modified by inertia, rather than being purely additive Thermal effects can help destabilize the plasma at long scales in the E‐region and at short scales in the F‐region</description><subject>Altitude</subject><subject>Altitude effects</subject><subject>Density</subject><subject>Density gradients</subject><subject>E region</subject><subject>F region</subject><subject>Instability</subject><subject>Ion thermal instability</subject><subject>Ionospheric plasma</subject><subject>Ionospheric propagation</subject><subject>Iterative methods</subject><subject>Magnetization</subject><subject>Magnetohydrodynamic stability</subject><subject>Nonisothermal processes</subject><subject>Plasma</subject><subject>Plasma instabilities</subject><subject>plasma instability</subject><subject>Polynomials</subject><subject>Propagation</subject><subject>Stability analysis</subject><subject>Temperature effects</subject><subject>thermal effects</subject><subject>Thermal instability</subject><subject>Wave propagation</subject><subject>Wavelengths</subject><issn>2169-9380</issn><issn>2169-9402</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2020</creationdate><recordtype>article</recordtype><recordid>eNp90cFOGzEQANAVAqko5dYPsMQ1Adu7NnZvqwBpEIgIRfS4mt2dTY02drANUXrqJ_Qf-mf9kjoNSDkxF4_GTx6NJ8u-MHrGKNfnnHJ6U1Ku8kIfZMecST3SBeWH73mu6KfsJIQnmkKlEhPH2Z-5W4NvSWnJ1EZceIjYkkeDa-I6MnXWhdUP9KYhsx7CEpIKEWrTm2gwfCXibIv-_vo9T2oJ_d79hnTOk9LXJnrwm60jd7CwGM1PiMbZIblEG7Zw4qE1aOOQgG3Jd3hFMvNuBYv_7nN21EEf8OTtHGTz66v5-Nvo9n4yHZe3oyYvhBxhLXPWdEp0da2KTspGK4pCImpoGG-7mhZaQtPymvNC1qkIshWKqwvGWpUPstPdsyvvnl8wxOrJvXibOla8EOnHNGM8qeFONd6F4LGrVt4s03wVo9V2EdX-IhLPd3xtetx8aKubyUMphL6Q-T_Ho4xi</recordid><startdate>202009</startdate><enddate>202009</enddate><creator>Makarevich, Roman A.</creator><general>Blackwell Publishing Ltd</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>8FD</scope><scope>H8D</scope><scope>KL.</scope><scope>L7M</scope><orcidid>https://orcid.org/0000-0002-4570-8948</orcidid></search><sort><creationdate>202009</creationdate><title>Toward An Integrated View of Ionospheric Plasma Instabilities: 5. 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Space physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Makarevich, Roman A.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Toward An Integrated View of Ionospheric Plasma Instabilities: 5. Ion‐Thermal Instability for Arbitrary Ion Magnetization, Density Gradient, and Wave Propagation</atitle><jtitle>Journal of geophysical research. Space physics</jtitle><date>2020-09</date><risdate>2020</risdate><volume>125</volume><issue>9</issue><epage>n/a</epage><issn>2169-9380</issn><eissn>2169-9402</eissn><abstract>A unified fluid theory of ionospheric electrostatic instabilities is presented that includes thermal effects due to nonisothermal processes for arbitrary ion magnetization, background density gradient, and wave propagation. 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At shorter wavelengths, they become comparable so that a significant fraction of propagation directions at λ=10 m have positive growth rates, in contrast with the isothermal FBI/GDI case, where stronger gradients are needed to destabilize the plasma at these short wavelengths. The overall conclusion is that the thermal effects modify the growth rate terms traditionally associated with FBI and GDI rather than being purely additive. Key Points Unified theory is developed for the ion‐thermal, Farley‐Buneman, and gradient‐drift instabilities for any magnetization and gradient Thermal effects modify the Farley‐Buneman and gradient‐drift factors, while being modified by inertia, rather than being purely additive Thermal effects can help destabilize the plasma at long scales in the E‐region and at short scales in the F‐region</abstract><cop>Washington</cop><pub>Blackwell Publishing Ltd</pub><doi>10.1029/2020JA028349</doi><tpages>20</tpages><orcidid>https://orcid.org/0000-0002-4570-8948</orcidid><oa>free_for_read</oa></addata></record>
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source Wiley-Blackwell Journals; Wiley Online Library Journals
subjects Altitude
Altitude effects
Density
Density gradients
E region
F region
Instability
Ion thermal instability
Ionospheric plasma
Ionospheric propagation
Iterative methods
Magnetization
Magnetohydrodynamic stability
Nonisothermal processes
Plasma
Plasma instabilities
plasma instability
Polynomials
Propagation
Stability analysis
Temperature effects
thermal effects
Thermal instability
Wave propagation
Wavelengths
title Toward An Integrated View of Ionospheric Plasma Instabilities: 5. Ion‐Thermal Instability for Arbitrary Ion Magnetization, Density Gradient, and Wave Propagation
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