On the Origin of High–Frequency Magnetic Fluctuations in the Interplanetary Medium: A Brownian–like Approach

Low–frequency fluctuations in the interplanetary medium have been extensively investigated and described in the framework of turbulence, and the observed universal scaling behavior represents a clear signature of the underlying energy cascade. On the contrary, the interpretation of observations of p...
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Autor*in:	Vincenzo Carbone [verfasserIn] Fabio Lepreti [verfasserIn] Antonio Vecchio [verfasserIn] Tommaso Alberti [verfasserIn] Federica Chiappetta [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2021

Schlagwörter:	Interplanetary medium interplanetary turbulence solar wind magnetic fields Heliosphere

Übergeordnetes Werk:	In: Frontiers in Physics - Frontiers Media S.A., 2014, 9(2021)
Übergeordnetes Werk:	volume:9 ; year:2021

Links:	Link aufrufen Link aufrufen Link aufrufen Journal toc

DOI / URN:	10.3389/fphy.2021.613759

Katalog-ID:	DOAJ062965492

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language	English
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container_title	Frontiers in Physics
authorswithroles_txt_mv	Vincenzo Carbone @@aut@@ Fabio Lepreti @@aut@@ Antonio Vecchio @@aut@@ Tommaso Alberti @@aut@@ Federica Chiappetta @@aut@@
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callnumber-first	Q - Science
author	Vincenzo Carbone
spellingShingle	Vincenzo Carbone misc QC1-999 misc Interplanetary medium misc interplanetary turbulence misc solar wind misc magnetic fields misc Heliosphere misc Physics On the Origin of High–Frequency Magnetic Fluctuations in the Interplanetary Medium: A Brownian–like Approach
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topic_title	QC1-999 On the Origin of High–Frequency Magnetic Fluctuations in the Interplanetary Medium: A Brownian–like Approach Interplanetary medium interplanetary turbulence solar wind magnetic fields Heliosphere
topic	misc QC1-999 misc Interplanetary medium misc interplanetary turbulence misc solar wind misc magnetic fields misc Heliosphere misc Physics
topic_unstemmed	misc QC1-999 misc Interplanetary medium misc interplanetary turbulence misc solar wind misc magnetic fields misc Heliosphere misc Physics
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title	On the Origin of High–Frequency Magnetic Fluctuations in the Interplanetary Medium: A Brownian–like Approach
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title_full	On the Origin of High–Frequency Magnetic Fluctuations in the Interplanetary Medium: A Brownian–like Approach
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title_sort	on the origin of high–frequency magnetic fluctuations in the interplanetary medium: a brownian–like approach
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title_auth	On the Origin of High–Frequency Magnetic Fluctuations in the Interplanetary Medium: A Brownian–like Approach
abstract	Low–frequency fluctuations in the interplanetary medium have been extensively investigated and described in the framework of turbulence, and the observed universal scaling behavior represents a clear signature of the underlying energy cascade. On the contrary, the interpretation of observations of plasma fluctuations at high frequencies, where wave–wave coupling, collisionless dissipation, and anomalous plasma heating play a key role, still represents a challenge for theoretical modeling. In this paper the high frequency fluctuations occurring in the interplanetary space are described through a Brownian–like approach, where the plasma dynamics at small scales is described through a stochastic process. It is shown that a simple model based on this framework is able to successfully reproduce the main features of the spectrum of the observed magnetic fluctuations. Moreover, the Fluctuation-Dissipation Relation, derived by our model, leads to a power law between dissipation rate and temperature, which is compatible with the occurrence of Landau damping, interpreted thus as the main mechanism of dissipation in the solar wind plasma.
abstractGer	Low–frequency fluctuations in the interplanetary medium have been extensively investigated and described in the framework of turbulence, and the observed universal scaling behavior represents a clear signature of the underlying energy cascade. On the contrary, the interpretation of observations of plasma fluctuations at high frequencies, where wave–wave coupling, collisionless dissipation, and anomalous plasma heating play a key role, still represents a challenge for theoretical modeling. In this paper the high frequency fluctuations occurring in the interplanetary space are described through a Brownian–like approach, where the plasma dynamics at small scales is described through a stochastic process. It is shown that a simple model based on this framework is able to successfully reproduce the main features of the spectrum of the observed magnetic fluctuations. Moreover, the Fluctuation-Dissipation Relation, derived by our model, leads to a power law between dissipation rate and temperature, which is compatible with the occurrence of Landau damping, interpreted thus as the main mechanism of dissipation in the solar wind plasma.
abstract_unstemmed	Low–frequency fluctuations in the interplanetary medium have been extensively investigated and described in the framework of turbulence, and the observed universal scaling behavior represents a clear signature of the underlying energy cascade. On the contrary, the interpretation of observations of plasma fluctuations at high frequencies, where wave–wave coupling, collisionless dissipation, and anomalous plasma heating play a key role, still represents a challenge for theoretical modeling. In this paper the high frequency fluctuations occurring in the interplanetary space are described through a Brownian–like approach, where the plasma dynamics at small scales is described through a stochastic process. It is shown that a simple model based on this framework is able to successfully reproduce the main features of the spectrum of the observed magnetic fluctuations. Moreover, the Fluctuation-Dissipation Relation, derived by our model, leads to a power law between dissipation rate and temperature, which is compatible with the occurrence of Landau damping, interpreted thus as the main mechanism of dissipation in the solar wind plasma.
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title_short	On the Origin of High–Frequency Magnetic Fluctuations in the Interplanetary Medium: A Brownian–like Approach
url	https://doi.org/10.3389/fphy.2021.613759 https://doaj.org/article/05a75774d1ff45d2bf0c08f0dcc9c19e https://www.frontiersin.org/articles/10.3389/fphy.2021.613759/full https://doaj.org/toc/2296-424X
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On the Origin of High–Frequency Magnetic Fluctuations in the Interplanetary Medium: A Brownian–like Approach

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