Turbulent dipolarization regions in the Earth’s magnetotail: ion fluxes and magnetic field changes

In this work, we consider the dynamics of ion fluxes and magnetic field changes in turbulent regions of magnetotail dipolarizations. The data from the Cluster-II mission (magnetic field measurements from fluxgate magnetometers and energetic charged particle observations from RAPID spectrometers) wer...

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Main Authors: Liudmyla Kozak, Elena A. Kronberg, Bohdan Petrenko, Aljona Blöcker, Roman Akhmetshyn, Istvan Ballai, Viktor Fedun
Format: Article
Language:English
Published: Frontiers Media S.A. 2023-10-01
Series:Frontiers in Astronomy and Space Sciences
Subjects:
Online Access:https://www.frontiersin.org/articles/10.3389/fspas.2023.1226200/full
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author Liudmyla Kozak
Liudmyla Kozak
Elena A. Kronberg
Bohdan Petrenko
Bohdan Petrenko
Aljona Blöcker
Roman Akhmetshyn
Istvan Ballai
Viktor Fedun
author_facet Liudmyla Kozak
Liudmyla Kozak
Elena A. Kronberg
Bohdan Petrenko
Bohdan Petrenko
Aljona Blöcker
Roman Akhmetshyn
Istvan Ballai
Viktor Fedun
author_sort Liudmyla Kozak
collection DOAJ
description In this work, we consider the dynamics of ion fluxes and magnetic field changes in turbulent regions of magnetotail dipolarizations. The data from the Cluster-II mission (magnetic field measurements from fluxgate magnetometers and energetic charged particle observations from RAPID spectrometers) were used for the analysis. We study individual events and investigate statistically the changes of charged particle fluxes during magnetic field dipolarizations observed during 2001–2015. Received changes in the spectral index indicate that CNO+ ions undergo stronger acceleration during dipolarization than protons and helium ions. Before dipolarization front monotonic growth the ions flux is observed (the maximum of flux is observed at 1–1,5 min after the start of dipolarization) in the range of ∼ 92–374 keV for proton; in the energy range ∼ 138–235 keV for He+ and in the energy range of 414–638 keV for CNO+ ions. Flux increase before arriving dipolarization front may result from the reflection of plasma sheet ions at the dipolarization front and the result of the resonant interactions of ions with low-frequency electromagnetic waves.
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spelling doaj.art-f21f7960254a4e8d8bf5b9e55fd51af52023-10-13T08:07:01ZengFrontiers Media S.A.Frontiers in Astronomy and Space Sciences2296-987X2023-10-011010.3389/fspas.2023.12262001226200Turbulent dipolarization regions in the Earth’s magnetotail: ion fluxes and magnetic field changesLiudmyla Kozak0Liudmyla Kozak1Elena A. Kronberg2Bohdan Petrenko3Bohdan Petrenko4Aljona Blöcker5Roman Akhmetshyn6Istvan Ballai7Viktor Fedun8Department Astronomy and Space Physics, Taras Shevchenko National University of Kyiv, Kyiv, UkraineSpace Research Institute of the National Academy of Sciences of Ukraine, The State Space Academy of Ukraine, Kyiv, UkraineGeophysics, Department of Earth and Environmental Sciences, University of Munich, Munich, GermanyDepartment Astronomy and Space Physics, Taras Shevchenko National University of Kyiv, Kyiv, UkraineSpace Research Institute of the National Academy of Sciences of Ukraine, The State Space Academy of Ukraine, Kyiv, UkraineGeophysics, Department of Earth and Environmental Sciences, University of Munich, Munich, GermanyDepartment Astronomy and Space Physics, Taras Shevchenko National University of Kyiv, Kyiv, UkrainePlasma Dynamics Group, School of Mathematics and Statistics, The University of Sheffield, Sheffield, United KingdomPlasma Dynamics Group, Department of Automatic Control and Systems Engineering, The University of Sheffield, Sheffield, United KingdomIn this work, we consider the dynamics of ion fluxes and magnetic field changes in turbulent regions of magnetotail dipolarizations. The data from the Cluster-II mission (magnetic field measurements from fluxgate magnetometers and energetic charged particle observations from RAPID spectrometers) were used for the analysis. We study individual events and investigate statistically the changes of charged particle fluxes during magnetic field dipolarizations observed during 2001–2015. Received changes in the spectral index indicate that CNO+ ions undergo stronger acceleration during dipolarization than protons and helium ions. Before dipolarization front monotonic growth the ions flux is observed (the maximum of flux is observed at 1–1,5 min after the start of dipolarization) in the range of ∼ 92–374 keV for proton; in the energy range ∼ 138–235 keV for He+ and in the energy range of 414–638 keV for CNO+ ions. Flux increase before arriving dipolarization front may result from the reflection of plasma sheet ions at the dipolarization front and the result of the resonant interactions of ions with low-frequency electromagnetic waves.https://www.frontiersin.org/articles/10.3389/fspas.2023.1226200/fulldipolarization frontscharged particlesdifferential fluxeswavessuperimposed epoch analysis
spellingShingle Liudmyla Kozak
Liudmyla Kozak
Elena A. Kronberg
Bohdan Petrenko
Bohdan Petrenko
Aljona Blöcker
Roman Akhmetshyn
Istvan Ballai
Viktor Fedun
Turbulent dipolarization regions in the Earth’s magnetotail: ion fluxes and magnetic field changes
Frontiers in Astronomy and Space Sciences
dipolarization fronts
charged particles
differential fluxes
waves
superimposed epoch analysis
title Turbulent dipolarization regions in the Earth’s magnetotail: ion fluxes and magnetic field changes
title_full Turbulent dipolarization regions in the Earth’s magnetotail: ion fluxes and magnetic field changes
title_fullStr Turbulent dipolarization regions in the Earth’s magnetotail: ion fluxes and magnetic field changes
title_full_unstemmed Turbulent dipolarization regions in the Earth’s magnetotail: ion fluxes and magnetic field changes
title_short Turbulent dipolarization regions in the Earth’s magnetotail: ion fluxes and magnetic field changes
title_sort turbulent dipolarization regions in the earth s magnetotail ion fluxes and magnetic field changes
topic dipolarization fronts
charged particles
differential fluxes
waves
superimposed epoch analysis
url https://www.frontiersin.org/articles/10.3389/fspas.2023.1226200/full
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