Energy Conversion through a Fluctuation–Dissipation Relation at Kinetic Scales in the Earth’s Magnetosheath

Low-frequency fluctuations in the interplanetary medium represent a turbulent environment where universal scaling behavior, generated by an energy cascade, has been investigated. On the contrary, in some regions, for example, the magnetosheath, universality of statistics of fluctuations is lost. How...
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Gespeichert in:

Autor*in:	Federica Chiappetta [verfasserIn] Emiliya Yordanova [verfasserIn] Zoltán Vörös [verfasserIn] Fabio Lepreti [verfasserIn] Vincenzo Carbone [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2023

Schlagwörter:	Interplanetary medium Heliosphere Space plasmas Interplanetary turbulence

Übergeordnetes Werk:	In: The Astrophysical Journal - IOP Publishing, 2022, 957(2023), 2, p 98
Übergeordnetes Werk:	volume:957 ; year:2023 ; number:2, p 98

Links:	Link aufrufen Link aufrufen Link aufrufen Journal toc

DOI / URN:	10.3847/1538-4357/acfca2

Katalog-ID:	DOAJ096872837

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language	English
source	In The Astrophysical Journal 957(2023), 2, p 98 volume:957 year:2023 number:2, p 98
sourceStr	In The Astrophysical Journal 957(2023), 2, p 98 volume:957 year:2023 number:2, p 98
format_phy_str_mv	Article
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topic_facet	Interplanetary medium Heliosphere Space plasmas Interplanetary turbulence Astrophysics
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container_title	The Astrophysical Journal
authorswithroles_txt_mv	Federica Chiappetta @@aut@@ Emiliya Yordanova @@aut@@ Zoltán Vörös @@aut@@ Fabio Lepreti @@aut@@ Vincenzo Carbone @@aut@@
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callnumber-first	Q - Science
author	Federica Chiappetta
spellingShingle	Federica Chiappetta misc QB460-466 misc Interplanetary medium misc Heliosphere misc Space plasmas misc Interplanetary turbulence misc Astrophysics Energy Conversion through a Fluctuation–Dissipation Relation at Kinetic Scales in the Earth’s Magnetosheath
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topic_title	QB460-466 Energy Conversion through a Fluctuation–Dissipation Relation at Kinetic Scales in the Earth’s Magnetosheath Interplanetary medium Heliosphere Space plasmas Interplanetary turbulence
topic	misc QB460-466 misc Interplanetary medium misc Heliosphere misc Space plasmas misc Interplanetary turbulence misc Astrophysics
topic_unstemmed	misc QB460-466 misc Interplanetary medium misc Heliosphere misc Space plasmas misc Interplanetary turbulence misc Astrophysics
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title	Energy Conversion through a Fluctuation–Dissipation Relation at Kinetic Scales in the Earth’s Magnetosheath
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title_sort	energy conversion through a fluctuation–dissipation relation at kinetic scales in the earth’s magnetosheath
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title_auth	Energy Conversion through a Fluctuation–Dissipation Relation at Kinetic Scales in the Earth’s Magnetosheath
abstract	Low-frequency fluctuations in the interplanetary medium represent a turbulent environment where universal scaling behavior, generated by an energy cascade, has been investigated. On the contrary, in some regions, for example, the magnetosheath, universality of statistics of fluctuations is lost. However, at kinetic scales where energy must be dissipated, the energy conversion seems to be realized through a mechanism similar to the free solar wind. Here we propose a Langevin model for magnetic fluctuations at kinetic scales, showing that the resulting fluctuation–dissipation relation is capable of describing the gross features of the spectral observations at kinetic scales in the magnetosheath. The fluctuation–dissipation relation regulates the energy conversion by imposing a relationship between fluctuations and dissipation, which at high frequencies are active at the same time in the same range of scales and represent two ingredients of the same physical process.
abstractGer	Low-frequency fluctuations in the interplanetary medium represent a turbulent environment where universal scaling behavior, generated by an energy cascade, has been investigated. On the contrary, in some regions, for example, the magnetosheath, universality of statistics of fluctuations is lost. However, at kinetic scales where energy must be dissipated, the energy conversion seems to be realized through a mechanism similar to the free solar wind. Here we propose a Langevin model for magnetic fluctuations at kinetic scales, showing that the resulting fluctuation–dissipation relation is capable of describing the gross features of the spectral observations at kinetic scales in the magnetosheath. The fluctuation–dissipation relation regulates the energy conversion by imposing a relationship between fluctuations and dissipation, which at high frequencies are active at the same time in the same range of scales and represent two ingredients of the same physical process.
abstract_unstemmed	Low-frequency fluctuations in the interplanetary medium represent a turbulent environment where universal scaling behavior, generated by an energy cascade, has been investigated. On the contrary, in some regions, for example, the magnetosheath, universality of statistics of fluctuations is lost. However, at kinetic scales where energy must be dissipated, the energy conversion seems to be realized through a mechanism similar to the free solar wind. Here we propose a Langevin model for magnetic fluctuations at kinetic scales, showing that the resulting fluctuation–dissipation relation is capable of describing the gross features of the spectral observations at kinetic scales in the magnetosheath. The fluctuation–dissipation relation regulates the energy conversion by imposing a relationship between fluctuations and dissipation, which at high frequencies are active at the same time in the same range of scales and represent two ingredients of the same physical process.
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title_short	Energy Conversion through a Fluctuation–Dissipation Relation at Kinetic Scales in the Earth’s Magnetosheath
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Energy Conversion through a Fluctuation–Dissipation Relation at Kinetic Scales in the Earth’s Magnetosheath

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