Pickup Ion–Mediated Magnetic Reconnection in the Outer Heliosphere

Pickup ions (PUIs) play a crucial role in the heliosphere, contributing to the mediation of large-scale structures such as the distant solar wind, the heliospheric termination shock, and the heliopause. While magnetic reconnection is thought to be a common process in the heliosphere due to the prese...
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Autor*in:	M. Nakanotani [verfasserIn] G. P. Zank [verfasserIn] L.-L. Zhao [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2023

Schlagwörter:	Heliosphere Solar magnetic reconnection Pickup ions

Übergeordnetes Werk:	In: The Astrophysical Journal Letters - IOP Publishing, 2022, 949(2023), 1, p L2
Übergeordnetes Werk:	volume:949 ; year:2023 ; number:1, p L2

Links:	Link aufrufen Link aufrufen Link aufrufen Journal toc

DOI / URN:	10.3847/2041-8213/acd33f

Katalog-ID:	DOAJ09058659X

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allfields	10.3847/2041-8213/acd33f doi (DE-627)DOAJ09058659X (DE-599)DOAJ6950aa6f40d24eb7b0d641551e12ec69 DE-627 ger DE-627 rakwb eng QB460-466 M. Nakanotani verfasserin aut Pickup Ion–Mediated Magnetic Reconnection in the Outer Heliosphere 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Pickup ions (PUIs) play a crucial role in the heliosphere, contributing to the mediation of large-scale structures such as the distant solar wind, the heliospheric termination shock, and the heliopause. While magnetic reconnection is thought to be a common process in the heliosphere due to the presence of heliospheric current sheets, it is poorly understood how PUIs might affect the evolution of magnetic reconnection. Although it is reasonable to suppose that PUIs decrease the reconnection rate since the plasma beta becomes much larger than 1 when PUIs are included, we show for the first time that such a supposition is invalid and that PUI-induced turbulence, heat conduction, and viscosity can preferentially boost magnetic reconnection in heliospheric current sheets in the distant solar wind. This suggests that it is critical to include the effect of the turbulence, heat conduction, and viscosity caused by PUIs to understand the dynamics of magnetic reconnection in the outer heliosphere. Heliosphere Solar magnetic reconnection Pickup ions Astrophysics G. P. Zank verfasserin aut L.-L. Zhao verfasserin aut In The Astrophysical Journal Letters IOP Publishing, 2022 949(2023), 1, p L2 (DE-627)312189028 (DE-600)2006858-X 20418213 nnns volume:949 year:2023 number:1, p L2 https://doi.org/10.3847/2041-8213/acd33f kostenfrei https://doaj.org/article/6950aa6f40d24eb7b0d641551e12ec69 kostenfrei https://doi.org/10.3847/2041-8213/acd33f kostenfrei https://doaj.org/toc/2041-8205 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ 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_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 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 949 2023 1, p L2
spelling	10.3847/2041-8213/acd33f doi (DE-627)DOAJ09058659X (DE-599)DOAJ6950aa6f40d24eb7b0d641551e12ec69 DE-627 ger DE-627 rakwb eng QB460-466 M. Nakanotani verfasserin aut Pickup Ion–Mediated Magnetic Reconnection in the Outer Heliosphere 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Pickup ions (PUIs) play a crucial role in the heliosphere, contributing to the mediation of large-scale structures such as the distant solar wind, the heliospheric termination shock, and the heliopause. While magnetic reconnection is thought to be a common process in the heliosphere due to the presence of heliospheric current sheets, it is poorly understood how PUIs might affect the evolution of magnetic reconnection. Although it is reasonable to suppose that PUIs decrease the reconnection rate since the plasma beta becomes much larger than 1 when PUIs are included, we show for the first time that such a supposition is invalid and that PUI-induced turbulence, heat conduction, and viscosity can preferentially boost magnetic reconnection in heliospheric current sheets in the distant solar wind. This suggests that it is critical to include the effect of the turbulence, heat conduction, and viscosity caused by PUIs to understand the dynamics of magnetic reconnection in the outer heliosphere. Heliosphere Solar magnetic reconnection Pickup ions Astrophysics G. P. Zank verfasserin aut L.-L. Zhao verfasserin aut In The Astrophysical Journal Letters IOP Publishing, 2022 949(2023), 1, p L2 (DE-627)312189028 (DE-600)2006858-X 20418213 nnns volume:949 year:2023 number:1, p L2 https://doi.org/10.3847/2041-8213/acd33f kostenfrei https://doaj.org/article/6950aa6f40d24eb7b0d641551e12ec69 kostenfrei https://doi.org/10.3847/2041-8213/acd33f kostenfrei https://doaj.org/toc/2041-8205 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ 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_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 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 949 2023 1, p L2
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allfieldsGer	10.3847/2041-8213/acd33f doi (DE-627)DOAJ09058659X (DE-599)DOAJ6950aa6f40d24eb7b0d641551e12ec69 DE-627 ger DE-627 rakwb eng QB460-466 M. Nakanotani verfasserin aut Pickup Ion–Mediated Magnetic Reconnection in the Outer Heliosphere 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Pickup ions (PUIs) play a crucial role in the heliosphere, contributing to the mediation of large-scale structures such as the distant solar wind, the heliospheric termination shock, and the heliopause. While magnetic reconnection is thought to be a common process in the heliosphere due to the presence of heliospheric current sheets, it is poorly understood how PUIs might affect the evolution of magnetic reconnection. Although it is reasonable to suppose that PUIs decrease the reconnection rate since the plasma beta becomes much larger than 1 when PUIs are included, we show for the first time that such a supposition is invalid and that PUI-induced turbulence, heat conduction, and viscosity can preferentially boost magnetic reconnection in heliospheric current sheets in the distant solar wind. This suggests that it is critical to include the effect of the turbulence, heat conduction, and viscosity caused by PUIs to understand the dynamics of magnetic reconnection in the outer heliosphere. Heliosphere Solar magnetic reconnection Pickup ions Astrophysics G. P. Zank verfasserin aut L.-L. Zhao verfasserin aut In The Astrophysical Journal Letters IOP Publishing, 2022 949(2023), 1, p L2 (DE-627)312189028 (DE-600)2006858-X 20418213 nnns volume:949 year:2023 number:1, p L2 https://doi.org/10.3847/2041-8213/acd33f kostenfrei https://doaj.org/article/6950aa6f40d24eb7b0d641551e12ec69 kostenfrei https://doi.org/10.3847/2041-8213/acd33f kostenfrei https://doaj.org/toc/2041-8205 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ 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_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 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 949 2023 1, p L2
allfieldsSound	10.3847/2041-8213/acd33f doi (DE-627)DOAJ09058659X (DE-599)DOAJ6950aa6f40d24eb7b0d641551e12ec69 DE-627 ger DE-627 rakwb eng QB460-466 M. Nakanotani verfasserin aut Pickup Ion–Mediated Magnetic Reconnection in the Outer Heliosphere 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Pickup ions (PUIs) play a crucial role in the heliosphere, contributing to the mediation of large-scale structures such as the distant solar wind, the heliospheric termination shock, and the heliopause. While magnetic reconnection is thought to be a common process in the heliosphere due to the presence of heliospheric current sheets, it is poorly understood how PUIs might affect the evolution of magnetic reconnection. Although it is reasonable to suppose that PUIs decrease the reconnection rate since the plasma beta becomes much larger than 1 when PUIs are included, we show for the first time that such a supposition is invalid and that PUI-induced turbulence, heat conduction, and viscosity can preferentially boost magnetic reconnection in heliospheric current sheets in the distant solar wind. This suggests that it is critical to include the effect of the turbulence, heat conduction, and viscosity caused by PUIs to understand the dynamics of magnetic reconnection in the outer heliosphere. Heliosphere Solar magnetic reconnection Pickup ions Astrophysics G. P. Zank verfasserin aut L.-L. Zhao verfasserin aut In The Astrophysical Journal Letters IOP Publishing, 2022 949(2023), 1, p L2 (DE-627)312189028 (DE-600)2006858-X 20418213 nnns volume:949 year:2023 number:1, p L2 https://doi.org/10.3847/2041-8213/acd33f kostenfrei https://doaj.org/article/6950aa6f40d24eb7b0d641551e12ec69 kostenfrei https://doi.org/10.3847/2041-8213/acd33f kostenfrei https://doaj.org/toc/2041-8205 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ 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_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 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 949 2023 1, p L2
language	English
source	In The Astrophysical Journal Letters 949(2023), 1, p L2 volume:949 year:2023 number:1, p L2
sourceStr	In The Astrophysical Journal Letters 949(2023), 1, p L2 volume:949 year:2023 number:1, p L2
format_phy_str_mv	Article
institution	findex.gbv.de
topic_facet	Heliosphere Solar magnetic reconnection Pickup ions Astrophysics
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container_title	The Astrophysical Journal Letters
authorswithroles_txt_mv	M. Nakanotani @@aut@@ G. P. Zank @@aut@@ L.-L. Zhao @@aut@@
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author	M. Nakanotani
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topic_title	QB460-466 Pickup Ion–Mediated Magnetic Reconnection in the Outer Heliosphere Heliosphere Solar magnetic reconnection Pickup ions
topic	misc QB460-466 misc Heliosphere misc Solar magnetic reconnection misc Pickup ions misc Astrophysics
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title_sort	pickup ion–mediated magnetic reconnection in the outer heliosphere
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title_auth	Pickup Ion–Mediated Magnetic Reconnection in the Outer Heliosphere
abstract	Pickup ions (PUIs) play a crucial role in the heliosphere, contributing to the mediation of large-scale structures such as the distant solar wind, the heliospheric termination shock, and the heliopause. While magnetic reconnection is thought to be a common process in the heliosphere due to the presence of heliospheric current sheets, it is poorly understood how PUIs might affect the evolution of magnetic reconnection. Although it is reasonable to suppose that PUIs decrease the reconnection rate since the plasma beta becomes much larger than 1 when PUIs are included, we show for the first time that such a supposition is invalid and that PUI-induced turbulence, heat conduction, and viscosity can preferentially boost magnetic reconnection in heliospheric current sheets in the distant solar wind. This suggests that it is critical to include the effect of the turbulence, heat conduction, and viscosity caused by PUIs to understand the dynamics of magnetic reconnection in the outer heliosphere.
abstractGer	Pickup ions (PUIs) play a crucial role in the heliosphere, contributing to the mediation of large-scale structures such as the distant solar wind, the heliospheric termination shock, and the heliopause. While magnetic reconnection is thought to be a common process in the heliosphere due to the presence of heliospheric current sheets, it is poorly understood how PUIs might affect the evolution of magnetic reconnection. Although it is reasonable to suppose that PUIs decrease the reconnection rate since the plasma beta becomes much larger than 1 when PUIs are included, we show for the first time that such a supposition is invalid and that PUI-induced turbulence, heat conduction, and viscosity can preferentially boost magnetic reconnection in heliospheric current sheets in the distant solar wind. This suggests that it is critical to include the effect of the turbulence, heat conduction, and viscosity caused by PUIs to understand the dynamics of magnetic reconnection in the outer heliosphere.
abstract_unstemmed	Pickup ions (PUIs) play a crucial role in the heliosphere, contributing to the mediation of large-scale structures such as the distant solar wind, the heliospheric termination shock, and the heliopause. While magnetic reconnection is thought to be a common process in the heliosphere due to the presence of heliospheric current sheets, it is poorly understood how PUIs might affect the evolution of magnetic reconnection. Although it is reasonable to suppose that PUIs decrease the reconnection rate since the plasma beta becomes much larger than 1 when PUIs are included, we show for the first time that such a supposition is invalid and that PUI-induced turbulence, heat conduction, and viscosity can preferentially boost magnetic reconnection in heliospheric current sheets in the distant solar wind. This suggests that it is critical to include the effect of the turbulence, heat conduction, and viscosity caused by PUIs to understand the dynamics of magnetic reconnection in the outer heliosphere.
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title_short	Pickup Ion–Mediated Magnetic Reconnection in the Outer Heliosphere
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Pickup Ion–Mediated Magnetic Reconnection in the Outer Heliosphere

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