Processes in auroral oval and outer electron radiation belt

Abstract We have analyzed the role of auroral processes in the formation of the outer radiation belt, considering that the main part of the auroral oval maps to the outer part of the ring current, instead of the plasma sheet as is commonly postulated. In this approach, the outer ring current is the...
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Autor*in:	Antonova, Elizaveta E. [verfasserIn] Stepanova, Marina V. Moya, Pablo S. Pinto, Victor A. Vovchenko, Vadim V. Ovchinnikov, Ilya L. Sotnikov, Nikita V.

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2018

Schlagwörter:	Magnetospheric storm and substorm Auroral oval Acceleration of electrons of the outer electron radiation belt

Anmerkung:	© The Author(s) 2018

Übergeordnetes Werk:	Enthalten in: Earth, planets and space - Heidelberg : Springer, 1998, 70(2018), 1 vom: 08. Aug.
Übergeordnetes Werk:	volume:70 ; year:2018 ; number:1 ; day:08 ; month:08

Links:	Volltext

DOI / URN:	10.1186/s40623-018-0898-1

Katalog-ID:	SPR036930075

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520			\|a Abstract We have analyzed the role of auroral processes in the formation of the outer radiation belt, considering that the main part of the auroral oval maps to the outer part of the ring current, instead of the plasma sheet as is commonly postulated. In this approach, the outer ring current is the region where transverse magnetospheric currents close inside the magnetosphere. Specifically, we analyzed the role of magnetospheric substorms in the appearance of relativistic electrons in the outer radiation belt. We present experimental evidence that the presence of substorms during a geomagnetic storm recovery phase is, in fact, very important for the appearance of a new radiation belt during this phase. We discuss the possible role of adiabatic acceleration of relativistic electrons during storm recovery phase and show that this mechanism may accelerate the relativistic electrons by more than one order of magnitude.
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allfields	10.1186/s40623-018-0898-1 doi (DE-627)SPR036930075 (SPR)s40623-018-0898-1-e DE-627 ger DE-627 rakwb eng Antonova, Elizaveta E. verfasserin (orcid)0000-0001-6980-3993 aut Processes in auroral oval and outer electron radiation belt 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2018 Abstract We have analyzed the role of auroral processes in the formation of the outer radiation belt, considering that the main part of the auroral oval maps to the outer part of the ring current, instead of the plasma sheet as is commonly postulated. In this approach, the outer ring current is the region where transverse magnetospheric currents close inside the magnetosphere. Specifically, we analyzed the role of magnetospheric substorms in the appearance of relativistic electrons in the outer radiation belt. We present experimental evidence that the presence of substorms during a geomagnetic storm recovery phase is, in fact, very important for the appearance of a new radiation belt during this phase. We discuss the possible role of adiabatic acceleration of relativistic electrons during storm recovery phase and show that this mechanism may accelerate the relativistic electrons by more than one order of magnitude. Magnetospheric storm and substorm (dpeaa)DE-He213 Auroral oval (dpeaa)DE-He213 Acceleration of electrons of the outer electron radiation belt (dpeaa)DE-He213 Stepanova, Marina V. aut Moya, Pablo S. aut Pinto, Victor A. aut Vovchenko, Vadim V. aut Ovchinnikov, Ilya L. aut Sotnikov, Nikita V. aut Enthalten in Earth, planets and space Heidelberg : Springer, 1998 70(2018), 1 vom: 08. Aug. (DE-627)353898597 (DE-600)2087663-4 1880-5981 nnns volume:70 year:2018 number:1 day:08 month:08 https://dx.doi.org/10.1186/s40623-018-0898-1 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 70 2018 1 08 08
spelling	10.1186/s40623-018-0898-1 doi (DE-627)SPR036930075 (SPR)s40623-018-0898-1-e DE-627 ger DE-627 rakwb eng Antonova, Elizaveta E. verfasserin (orcid)0000-0001-6980-3993 aut Processes in auroral oval and outer electron radiation belt 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2018 Abstract We have analyzed the role of auroral processes in the formation of the outer radiation belt, considering that the main part of the auroral oval maps to the outer part of the ring current, instead of the plasma sheet as is commonly postulated. In this approach, the outer ring current is the region where transverse magnetospheric currents close inside the magnetosphere. Specifically, we analyzed the role of magnetospheric substorms in the appearance of relativistic electrons in the outer radiation belt. We present experimental evidence that the presence of substorms during a geomagnetic storm recovery phase is, in fact, very important for the appearance of a new radiation belt during this phase. We discuss the possible role of adiabatic acceleration of relativistic electrons during storm recovery phase and show that this mechanism may accelerate the relativistic electrons by more than one order of magnitude. Magnetospheric storm and substorm (dpeaa)DE-He213 Auroral oval (dpeaa)DE-He213 Acceleration of electrons of the outer electron radiation belt (dpeaa)DE-He213 Stepanova, Marina V. aut Moya, Pablo S. aut Pinto, Victor A. aut Vovchenko, Vadim V. aut Ovchinnikov, Ilya L. aut Sotnikov, Nikita V. aut Enthalten in Earth, planets and space Heidelberg : Springer, 1998 70(2018), 1 vom: 08. Aug. (DE-627)353898597 (DE-600)2087663-4 1880-5981 nnns volume:70 year:2018 number:1 day:08 month:08 https://dx.doi.org/10.1186/s40623-018-0898-1 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 70 2018 1 08 08
allfields_unstemmed	10.1186/s40623-018-0898-1 doi (DE-627)SPR036930075 (SPR)s40623-018-0898-1-e DE-627 ger DE-627 rakwb eng Antonova, Elizaveta E. verfasserin (orcid)0000-0001-6980-3993 aut Processes in auroral oval and outer electron radiation belt 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2018 Abstract We have analyzed the role of auroral processes in the formation of the outer radiation belt, considering that the main part of the auroral oval maps to the outer part of the ring current, instead of the plasma sheet as is commonly postulated. In this approach, the outer ring current is the region where transverse magnetospheric currents close inside the magnetosphere. Specifically, we analyzed the role of magnetospheric substorms in the appearance of relativistic electrons in the outer radiation belt. We present experimental evidence that the presence of substorms during a geomagnetic storm recovery phase is, in fact, very important for the appearance of a new radiation belt during this phase. We discuss the possible role of adiabatic acceleration of relativistic electrons during storm recovery phase and show that this mechanism may accelerate the relativistic electrons by more than one order of magnitude. Magnetospheric storm and substorm (dpeaa)DE-He213 Auroral oval (dpeaa)DE-He213 Acceleration of electrons of the outer electron radiation belt (dpeaa)DE-He213 Stepanova, Marina V. aut Moya, Pablo S. aut Pinto, Victor A. aut Vovchenko, Vadim V. aut Ovchinnikov, Ilya L. aut Sotnikov, Nikita V. aut Enthalten in Earth, planets and space Heidelberg : Springer, 1998 70(2018), 1 vom: 08. Aug. (DE-627)353898597 (DE-600)2087663-4 1880-5981 nnns volume:70 year:2018 number:1 day:08 month:08 https://dx.doi.org/10.1186/s40623-018-0898-1 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 70 2018 1 08 08
allfieldsGer	10.1186/s40623-018-0898-1 doi (DE-627)SPR036930075 (SPR)s40623-018-0898-1-e DE-627 ger DE-627 rakwb eng Antonova, Elizaveta E. verfasserin (orcid)0000-0001-6980-3993 aut Processes in auroral oval and outer electron radiation belt 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2018 Abstract We have analyzed the role of auroral processes in the formation of the outer radiation belt, considering that the main part of the auroral oval maps to the outer part of the ring current, instead of the plasma sheet as is commonly postulated. In this approach, the outer ring current is the region where transverse magnetospheric currents close inside the magnetosphere. Specifically, we analyzed the role of magnetospheric substorms in the appearance of relativistic electrons in the outer radiation belt. We present experimental evidence that the presence of substorms during a geomagnetic storm recovery phase is, in fact, very important for the appearance of a new radiation belt during this phase. We discuss the possible role of adiabatic acceleration of relativistic electrons during storm recovery phase and show that this mechanism may accelerate the relativistic electrons by more than one order of magnitude. Magnetospheric storm and substorm (dpeaa)DE-He213 Auroral oval (dpeaa)DE-He213 Acceleration of electrons of the outer electron radiation belt (dpeaa)DE-He213 Stepanova, Marina V. aut Moya, Pablo S. aut Pinto, Victor A. aut Vovchenko, Vadim V. aut Ovchinnikov, Ilya L. aut Sotnikov, Nikita V. aut Enthalten in Earth, planets and space Heidelberg : Springer, 1998 70(2018), 1 vom: 08. Aug. (DE-627)353898597 (DE-600)2087663-4 1880-5981 nnns volume:70 year:2018 number:1 day:08 month:08 https://dx.doi.org/10.1186/s40623-018-0898-1 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 70 2018 1 08 08
allfieldsSound	10.1186/s40623-018-0898-1 doi (DE-627)SPR036930075 (SPR)s40623-018-0898-1-e DE-627 ger DE-627 rakwb eng Antonova, Elizaveta E. verfasserin (orcid)0000-0001-6980-3993 aut Processes in auroral oval and outer electron radiation belt 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2018 Abstract We have analyzed the role of auroral processes in the formation of the outer radiation belt, considering that the main part of the auroral oval maps to the outer part of the ring current, instead of the plasma sheet as is commonly postulated. In this approach, the outer ring current is the region where transverse magnetospheric currents close inside the magnetosphere. Specifically, we analyzed the role of magnetospheric substorms in the appearance of relativistic electrons in the outer radiation belt. We present experimental evidence that the presence of substorms during a geomagnetic storm recovery phase is, in fact, very important for the appearance of a new radiation belt during this phase. We discuss the possible role of adiabatic acceleration of relativistic electrons during storm recovery phase and show that this mechanism may accelerate the relativistic electrons by more than one order of magnitude. Magnetospheric storm and substorm (dpeaa)DE-He213 Auroral oval (dpeaa)DE-He213 Acceleration of electrons of the outer electron radiation belt (dpeaa)DE-He213 Stepanova, Marina V. aut Moya, Pablo S. aut Pinto, Victor A. aut Vovchenko, Vadim V. aut Ovchinnikov, Ilya L. aut Sotnikov, Nikita V. aut Enthalten in Earth, planets and space Heidelberg : Springer, 1998 70(2018), 1 vom: 08. Aug. (DE-627)353898597 (DE-600)2087663-4 1880-5981 nnns volume:70 year:2018 number:1 day:08 month:08 https://dx.doi.org/10.1186/s40623-018-0898-1 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 70 2018 1 08 08
language	English
source	Enthalten in Earth, planets and space 70(2018), 1 vom: 08. Aug. volume:70 year:2018 number:1 day:08 month:08
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topic_facet	Magnetospheric storm and substorm Auroral oval Acceleration of electrons of the outer electron radiation belt
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author	Antonova, Elizaveta E.
spellingShingle	Antonova, Elizaveta E. misc Magnetospheric storm and substorm misc Auroral oval misc Acceleration of electrons of the outer electron radiation belt Processes in auroral oval and outer electron radiation belt
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topic_title	Processes in auroral oval and outer electron radiation belt Magnetospheric storm and substorm (dpeaa)DE-He213 Auroral oval (dpeaa)DE-He213 Acceleration of electrons of the outer electron radiation belt (dpeaa)DE-He213
topic	misc Magnetospheric storm and substorm misc Auroral oval misc Acceleration of electrons of the outer electron radiation belt
topic_unstemmed	misc Magnetospheric storm and substorm misc Auroral oval misc Acceleration of electrons of the outer electron radiation belt
topic_browse	misc Magnetospheric storm and substorm misc Auroral oval misc Acceleration of electrons of the outer electron radiation belt
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title	Processes in auroral oval and outer electron radiation belt
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title_full	Processes in auroral oval and outer electron radiation belt
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author_browse	Antonova, Elizaveta E. Stepanova, Marina V. Moya, Pablo S. Pinto, Victor A. Vovchenko, Vadim V. Ovchinnikov, Ilya L. Sotnikov, Nikita V.
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title_sort	processes in auroral oval and outer electron radiation belt
title_auth	Processes in auroral oval and outer electron radiation belt
abstract	Abstract We have analyzed the role of auroral processes in the formation of the outer radiation belt, considering that the main part of the auroral oval maps to the outer part of the ring current, instead of the plasma sheet as is commonly postulated. In this approach, the outer ring current is the region where transverse magnetospheric currents close inside the magnetosphere. Specifically, we analyzed the role of magnetospheric substorms in the appearance of relativistic electrons in the outer radiation belt. We present experimental evidence that the presence of substorms during a geomagnetic storm recovery phase is, in fact, very important for the appearance of a new radiation belt during this phase. We discuss the possible role of adiabatic acceleration of relativistic electrons during storm recovery phase and show that this mechanism may accelerate the relativistic electrons by more than one order of magnitude. © The Author(s) 2018
abstractGer	Abstract We have analyzed the role of auroral processes in the formation of the outer radiation belt, considering that the main part of the auroral oval maps to the outer part of the ring current, instead of the plasma sheet as is commonly postulated. In this approach, the outer ring current is the region where transverse magnetospheric currents close inside the magnetosphere. Specifically, we analyzed the role of magnetospheric substorms in the appearance of relativistic electrons in the outer radiation belt. We present experimental evidence that the presence of substorms during a geomagnetic storm recovery phase is, in fact, very important for the appearance of a new radiation belt during this phase. We discuss the possible role of adiabatic acceleration of relativistic electrons during storm recovery phase and show that this mechanism may accelerate the relativistic electrons by more than one order of magnitude. © The Author(s) 2018
abstract_unstemmed	Abstract We have analyzed the role of auroral processes in the formation of the outer radiation belt, considering that the main part of the auroral oval maps to the outer part of the ring current, instead of the plasma sheet as is commonly postulated. In this approach, the outer ring current is the region where transverse magnetospheric currents close inside the magnetosphere. Specifically, we analyzed the role of magnetospheric substorms in the appearance of relativistic electrons in the outer radiation belt. We present experimental evidence that the presence of substorms during a geomagnetic storm recovery phase is, in fact, very important for the appearance of a new radiation belt during this phase. We discuss the possible role of adiabatic acceleration of relativistic electrons during storm recovery phase and show that this mechanism may accelerate the relativistic electrons by more than one order of magnitude. © The Author(s) 2018
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title_short	Processes in auroral oval and outer electron radiation belt
url	https://dx.doi.org/10.1186/s40623-018-0898-1
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author2	Stepanova, Marina V. Moya, Pablo S. Pinto, Victor A. Vovchenko, Vadim V. Ovchinnikov, Ilya L. Sotnikov, Nikita V.
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Processes in auroral oval and outer electron radiation belt

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Vorhandene Bände

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