Variation of dayside chorus waves associated with solar wind dynamic pressure based on MMS observations
The whistler-mode chorus waves are one of the most important plasma waves in the Earth’s magnetosphere. Generally, the amplitude of whistler-mode chorus waves prefers to strengthen when the energetic fluxes of anisotropic electrons increase outside the plasmapause. This characteristic is commonly as...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Peng, Qianshui [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2020transfer abstract |
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| Schlagwörter: |
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| Umfang: |
8 |
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| Übergeordnetes Werk: |
Enthalten in: Posttranscriptional actions of triiodothyronine on - Bargi-Souza, Paula ELSEVIER, 2018, including COSPAR information bulletin : the official journal of the Committee on Space Research (COSPAR), a scientific committee of the International Council of Scientific Unions (ICSU), Amsterdam [u.a.] |
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| Übergeordnetes Werk: |
volume:65 ; year:2020 ; number:11 ; day:1 ; month:06 ; pages:2551-2558 ; extent:8 |
| Links: |
|---|
| DOI / URN: |
10.1016/j.asr.2020.03.006 |
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ELV05009842X |
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| 245 | 1 | 0 | |a Variation of dayside chorus waves associated with solar wind dynamic pressure based on MMS observations |
| 264 | 1 | |c 2020transfer abstract | |
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| 520 | |a The whistler-mode chorus waves are one of the most important plasma waves in the Earth’s magnetosphere. Generally, the amplitude of whistler-mode chorus waves prefers to strengthen when the energetic fluxes of anisotropic electrons increase outside the plasmapause. This characteristic is commonly associated with the geomagnetic storms or substorms. However, the relationship between the solar wind dynamic pressure (P sw) and the long-time variation of chorus waves during the quiet period of the geomagnetic activity still needs more detailed investigations. In this paper, based on MMS observations, we present a chorus event just observed in the inner side of magnetopause without obvious geomagnetic storms or substroms. Interestingly, during this time interval, some P sw fluctuations were recorded. Both the amplitudes and frequencies of chorus waves changed as a response to the variation in P sw. It proved that the enhancement of P sw increases the energetic electrons fluxes, which provides free energies for the chorus amplification. Furthermore, the wave growth rates calculated using linear theory increases and the central frequency of the chorus waves shifts to a higher frequency when the P sw enhancement is greater, which are also consistent well with the observations. The results provide a direct evidence that the P sw play an important role in the long-time variation of whistler-mode chorus waves inside the magnetopause. | ||
| 520 | |a The whistler-mode chorus waves are one of the most important plasma waves in the Earth’s magnetosphere. Generally, the amplitude of whistler-mode chorus waves prefers to strengthen when the energetic fluxes of anisotropic electrons increase outside the plasmapause. This characteristic is commonly associated with the geomagnetic storms or substorms. However, the relationship between the solar wind dynamic pressure (P sw) and the long-time variation of chorus waves during the quiet period of the geomagnetic activity still needs more detailed investigations. In this paper, based on MMS observations, we present a chorus event just observed in the inner side of magnetopause without obvious geomagnetic storms or substroms. Interestingly, during this time interval, some P sw fluctuations were recorded. Both the amplitudes and frequencies of chorus waves changed as a response to the variation in P sw. It proved that the enhancement of P sw increases the energetic electrons fluxes, which provides free energies for the chorus amplification. Furthermore, the wave growth rates calculated using linear theory increases and the central frequency of the chorus waves shifts to a higher frequency when the P sw enhancement is greater, which are also consistent well with the observations. The results provide a direct evidence that the P sw play an important role in the long-time variation of whistler-mode chorus waves inside the magnetopause. | ||
| 650 | 7 | |a Energetic electron flux |2 Elsevier | |
| 650 | 7 | |a Whistler-mode chorus waves |2 Elsevier | |
| 650 | 7 | |a Wave-particle interaction |2 Elsevier | |
| 650 | 7 | |a Solar wind |2 Elsevier | |
| 700 | 1 | |a Li, Haimeng |4 oth | |
| 700 | 1 | |a Tang, Rongxin |4 oth | |
| 700 | 1 | |a Zhong, Zhihong |4 oth | |
| 700 | 1 | |a Zhang, He |4 oth | |
| 700 | 1 | |a Li, Qiang |4 oth | |
| 773 | 0 | 8 | |i Enthalten in |n Elsevier Science |a Bargi-Souza, Paula ELSEVIER |t Posttranscriptional actions of triiodothyronine on |d 2018 |d including COSPAR information bulletin : the official journal of the Committee on Space Research (COSPAR), a scientific committee of the International Council of Scientific Unions (ICSU) |g Amsterdam [u.a.] |w (DE-627)ELV000905844 |
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10.1016/j.asr.2020.03.006 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000000988.pica (DE-627)ELV05009842X (ELSEVIER)S0273-1177(20)30145-9 DE-627 ger DE-627 rakwb eng 610 570 VZ 44.89 bkl Peng, Qianshui verfasserin aut Variation of dayside chorus waves associated with solar wind dynamic pressure based on MMS observations 2020transfer abstract 8 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The whistler-mode chorus waves are one of the most important plasma waves in the Earth’s magnetosphere. Generally, the amplitude of whistler-mode chorus waves prefers to strengthen when the energetic fluxes of anisotropic electrons increase outside the plasmapause. This characteristic is commonly associated with the geomagnetic storms or substorms. However, the relationship between the solar wind dynamic pressure (P sw) and the long-time variation of chorus waves during the quiet period of the geomagnetic activity still needs more detailed investigations. In this paper, based on MMS observations, we present a chorus event just observed in the inner side of magnetopause without obvious geomagnetic storms or substroms. Interestingly, during this time interval, some P sw fluctuations were recorded. Both the amplitudes and frequencies of chorus waves changed as a response to the variation in P sw. It proved that the enhancement of P sw increases the energetic electrons fluxes, which provides free energies for the chorus amplification. Furthermore, the wave growth rates calculated using linear theory increases and the central frequency of the chorus waves shifts to a higher frequency when the P sw enhancement is greater, which are also consistent well with the observations. The results provide a direct evidence that the P sw play an important role in the long-time variation of whistler-mode chorus waves inside the magnetopause. The whistler-mode chorus waves are one of the most important plasma waves in the Earth’s magnetosphere. Generally, the amplitude of whistler-mode chorus waves prefers to strengthen when the energetic fluxes of anisotropic electrons increase outside the plasmapause. This characteristic is commonly associated with the geomagnetic storms or substorms. However, the relationship between the solar wind dynamic pressure (P sw) and the long-time variation of chorus waves during the quiet period of the geomagnetic activity still needs more detailed investigations. In this paper, based on MMS observations, we present a chorus event just observed in the inner side of magnetopause without obvious geomagnetic storms or substroms. Interestingly, during this time interval, some P sw fluctuations were recorded. Both the amplitudes and frequencies of chorus waves changed as a response to the variation in P sw. It proved that the enhancement of P sw increases the energetic electrons fluxes, which provides free energies for the chorus amplification. Furthermore, the wave growth rates calculated using linear theory increases and the central frequency of the chorus waves shifts to a higher frequency when the P sw enhancement is greater, which are also consistent well with the observations. The results provide a direct evidence that the P sw play an important role in the long-time variation of whistler-mode chorus waves inside the magnetopause. Energetic electron flux Elsevier Whistler-mode chorus waves Elsevier Wave-particle interaction Elsevier Solar wind Elsevier Li, Haimeng oth Tang, Rongxin oth Zhong, Zhihong oth Zhang, He oth Li, Qiang oth Enthalten in Elsevier Science Bargi-Souza, Paula ELSEVIER Posttranscriptional actions of triiodothyronine on 2018 including COSPAR information bulletin : the official journal of the Committee on Space Research (COSPAR), a scientific committee of the International Council of Scientific Unions (ICSU) Amsterdam [u.a.] (DE-627)ELV000905844 volume:65 year:2020 number:11 day:1 month:06 pages:2551-2558 extent:8 https://doi.org/10.1016/j.asr.2020.03.006 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA 44.89 Endokrinologie VZ AR 65 2020 11 1 0601 2551-2558 8 |
| spelling |
10.1016/j.asr.2020.03.006 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000000988.pica (DE-627)ELV05009842X (ELSEVIER)S0273-1177(20)30145-9 DE-627 ger DE-627 rakwb eng 610 570 VZ 44.89 bkl Peng, Qianshui verfasserin aut Variation of dayside chorus waves associated with solar wind dynamic pressure based on MMS observations 2020transfer abstract 8 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The whistler-mode chorus waves are one of the most important plasma waves in the Earth’s magnetosphere. Generally, the amplitude of whistler-mode chorus waves prefers to strengthen when the energetic fluxes of anisotropic electrons increase outside the plasmapause. This characteristic is commonly associated with the geomagnetic storms or substorms. However, the relationship between the solar wind dynamic pressure (P sw) and the long-time variation of chorus waves during the quiet period of the geomagnetic activity still needs more detailed investigations. In this paper, based on MMS observations, we present a chorus event just observed in the inner side of magnetopause without obvious geomagnetic storms or substroms. Interestingly, during this time interval, some P sw fluctuations were recorded. Both the amplitudes and frequencies of chorus waves changed as a response to the variation in P sw. It proved that the enhancement of P sw increases the energetic electrons fluxes, which provides free energies for the chorus amplification. Furthermore, the wave growth rates calculated using linear theory increases and the central frequency of the chorus waves shifts to a higher frequency when the P sw enhancement is greater, which are also consistent well with the observations. The results provide a direct evidence that the P sw play an important role in the long-time variation of whistler-mode chorus waves inside the magnetopause. The whistler-mode chorus waves are one of the most important plasma waves in the Earth’s magnetosphere. Generally, the amplitude of whistler-mode chorus waves prefers to strengthen when the energetic fluxes of anisotropic electrons increase outside the plasmapause. This characteristic is commonly associated with the geomagnetic storms or substorms. However, the relationship between the solar wind dynamic pressure (P sw) and the long-time variation of chorus waves during the quiet period of the geomagnetic activity still needs more detailed investigations. In this paper, based on MMS observations, we present a chorus event just observed in the inner side of magnetopause without obvious geomagnetic storms or substroms. Interestingly, during this time interval, some P sw fluctuations were recorded. Both the amplitudes and frequencies of chorus waves changed as a response to the variation in P sw. It proved that the enhancement of P sw increases the energetic electrons fluxes, which provides free energies for the chorus amplification. Furthermore, the wave growth rates calculated using linear theory increases and the central frequency of the chorus waves shifts to a higher frequency when the P sw enhancement is greater, which are also consistent well with the observations. The results provide a direct evidence that the P sw play an important role in the long-time variation of whistler-mode chorus waves inside the magnetopause. Energetic electron flux Elsevier Whistler-mode chorus waves Elsevier Wave-particle interaction Elsevier Solar wind Elsevier Li, Haimeng oth Tang, Rongxin oth Zhong, Zhihong oth Zhang, He oth Li, Qiang oth Enthalten in Elsevier Science Bargi-Souza, Paula ELSEVIER Posttranscriptional actions of triiodothyronine on 2018 including COSPAR information bulletin : the official journal of the Committee on Space Research (COSPAR), a scientific committee of the International Council of Scientific Unions (ICSU) Amsterdam [u.a.] (DE-627)ELV000905844 volume:65 year:2020 number:11 day:1 month:06 pages:2551-2558 extent:8 https://doi.org/10.1016/j.asr.2020.03.006 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA 44.89 Endokrinologie VZ AR 65 2020 11 1 0601 2551-2558 8 |
| allfields_unstemmed |
10.1016/j.asr.2020.03.006 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000000988.pica (DE-627)ELV05009842X (ELSEVIER)S0273-1177(20)30145-9 DE-627 ger DE-627 rakwb eng 610 570 VZ 44.89 bkl Peng, Qianshui verfasserin aut Variation of dayside chorus waves associated with solar wind dynamic pressure based on MMS observations 2020transfer abstract 8 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The whistler-mode chorus waves are one of the most important plasma waves in the Earth’s magnetosphere. Generally, the amplitude of whistler-mode chorus waves prefers to strengthen when the energetic fluxes of anisotropic electrons increase outside the plasmapause. This characteristic is commonly associated with the geomagnetic storms or substorms. However, the relationship between the solar wind dynamic pressure (P sw) and the long-time variation of chorus waves during the quiet period of the geomagnetic activity still needs more detailed investigations. In this paper, based on MMS observations, we present a chorus event just observed in the inner side of magnetopause without obvious geomagnetic storms or substroms. Interestingly, during this time interval, some P sw fluctuations were recorded. Both the amplitudes and frequencies of chorus waves changed as a response to the variation in P sw. It proved that the enhancement of P sw increases the energetic electrons fluxes, which provides free energies for the chorus amplification. Furthermore, the wave growth rates calculated using linear theory increases and the central frequency of the chorus waves shifts to a higher frequency when the P sw enhancement is greater, which are also consistent well with the observations. The results provide a direct evidence that the P sw play an important role in the long-time variation of whistler-mode chorus waves inside the magnetopause. The whistler-mode chorus waves are one of the most important plasma waves in the Earth’s magnetosphere. Generally, the amplitude of whistler-mode chorus waves prefers to strengthen when the energetic fluxes of anisotropic electrons increase outside the plasmapause. This characteristic is commonly associated with the geomagnetic storms or substorms. However, the relationship between the solar wind dynamic pressure (P sw) and the long-time variation of chorus waves during the quiet period of the geomagnetic activity still needs more detailed investigations. In this paper, based on MMS observations, we present a chorus event just observed in the inner side of magnetopause without obvious geomagnetic storms or substroms. Interestingly, during this time interval, some P sw fluctuations were recorded. Both the amplitudes and frequencies of chorus waves changed as a response to the variation in P sw. It proved that the enhancement of P sw increases the energetic electrons fluxes, which provides free energies for the chorus amplification. Furthermore, the wave growth rates calculated using linear theory increases and the central frequency of the chorus waves shifts to a higher frequency when the P sw enhancement is greater, which are also consistent well with the observations. The results provide a direct evidence that the P sw play an important role in the long-time variation of whistler-mode chorus waves inside the magnetopause. Energetic electron flux Elsevier Whistler-mode chorus waves Elsevier Wave-particle interaction Elsevier Solar wind Elsevier Li, Haimeng oth Tang, Rongxin oth Zhong, Zhihong oth Zhang, He oth Li, Qiang oth Enthalten in Elsevier Science Bargi-Souza, Paula ELSEVIER Posttranscriptional actions of triiodothyronine on 2018 including COSPAR information bulletin : the official journal of the Committee on Space Research (COSPAR), a scientific committee of the International Council of Scientific Unions (ICSU) Amsterdam [u.a.] (DE-627)ELV000905844 volume:65 year:2020 number:11 day:1 month:06 pages:2551-2558 extent:8 https://doi.org/10.1016/j.asr.2020.03.006 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA 44.89 Endokrinologie VZ AR 65 2020 11 1 0601 2551-2558 8 |
| allfieldsGer |
10.1016/j.asr.2020.03.006 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000000988.pica (DE-627)ELV05009842X (ELSEVIER)S0273-1177(20)30145-9 DE-627 ger DE-627 rakwb eng 610 570 VZ 44.89 bkl Peng, Qianshui verfasserin aut Variation of dayside chorus waves associated with solar wind dynamic pressure based on MMS observations 2020transfer abstract 8 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The whistler-mode chorus waves are one of the most important plasma waves in the Earth’s magnetosphere. Generally, the amplitude of whistler-mode chorus waves prefers to strengthen when the energetic fluxes of anisotropic electrons increase outside the plasmapause. This characteristic is commonly associated with the geomagnetic storms or substorms. However, the relationship between the solar wind dynamic pressure (P sw) and the long-time variation of chorus waves during the quiet period of the geomagnetic activity still needs more detailed investigations. In this paper, based on MMS observations, we present a chorus event just observed in the inner side of magnetopause without obvious geomagnetic storms or substroms. Interestingly, during this time interval, some P sw fluctuations were recorded. Both the amplitudes and frequencies of chorus waves changed as a response to the variation in P sw. It proved that the enhancement of P sw increases the energetic electrons fluxes, which provides free energies for the chorus amplification. Furthermore, the wave growth rates calculated using linear theory increases and the central frequency of the chorus waves shifts to a higher frequency when the P sw enhancement is greater, which are also consistent well with the observations. The results provide a direct evidence that the P sw play an important role in the long-time variation of whistler-mode chorus waves inside the magnetopause. The whistler-mode chorus waves are one of the most important plasma waves in the Earth’s magnetosphere. Generally, the amplitude of whistler-mode chorus waves prefers to strengthen when the energetic fluxes of anisotropic electrons increase outside the plasmapause. This characteristic is commonly associated with the geomagnetic storms or substorms. However, the relationship between the solar wind dynamic pressure (P sw) and the long-time variation of chorus waves during the quiet period of the geomagnetic activity still needs more detailed investigations. In this paper, based on MMS observations, we present a chorus event just observed in the inner side of magnetopause without obvious geomagnetic storms or substroms. Interestingly, during this time interval, some P sw fluctuations were recorded. Both the amplitudes and frequencies of chorus waves changed as a response to the variation in P sw. It proved that the enhancement of P sw increases the energetic electrons fluxes, which provides free energies for the chorus amplification. Furthermore, the wave growth rates calculated using linear theory increases and the central frequency of the chorus waves shifts to a higher frequency when the P sw enhancement is greater, which are also consistent well with the observations. The results provide a direct evidence that the P sw play an important role in the long-time variation of whistler-mode chorus waves inside the magnetopause. Energetic electron flux Elsevier Whistler-mode chorus waves Elsevier Wave-particle interaction Elsevier Solar wind Elsevier Li, Haimeng oth Tang, Rongxin oth Zhong, Zhihong oth Zhang, He oth Li, Qiang oth Enthalten in Elsevier Science Bargi-Souza, Paula ELSEVIER Posttranscriptional actions of triiodothyronine on 2018 including COSPAR information bulletin : the official journal of the Committee on Space Research (COSPAR), a scientific committee of the International Council of Scientific Unions (ICSU) Amsterdam [u.a.] (DE-627)ELV000905844 volume:65 year:2020 number:11 day:1 month:06 pages:2551-2558 extent:8 https://doi.org/10.1016/j.asr.2020.03.006 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA 44.89 Endokrinologie VZ AR 65 2020 11 1 0601 2551-2558 8 |
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10.1016/j.asr.2020.03.006 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000000988.pica (DE-627)ELV05009842X (ELSEVIER)S0273-1177(20)30145-9 DE-627 ger DE-627 rakwb eng 610 570 VZ 44.89 bkl Peng, Qianshui verfasserin aut Variation of dayside chorus waves associated with solar wind dynamic pressure based on MMS observations 2020transfer abstract 8 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The whistler-mode chorus waves are one of the most important plasma waves in the Earth’s magnetosphere. Generally, the amplitude of whistler-mode chorus waves prefers to strengthen when the energetic fluxes of anisotropic electrons increase outside the plasmapause. This characteristic is commonly associated with the geomagnetic storms or substorms. However, the relationship between the solar wind dynamic pressure (P sw) and the long-time variation of chorus waves during the quiet period of the geomagnetic activity still needs more detailed investigations. In this paper, based on MMS observations, we present a chorus event just observed in the inner side of magnetopause without obvious geomagnetic storms or substroms. Interestingly, during this time interval, some P sw fluctuations were recorded. Both the amplitudes and frequencies of chorus waves changed as a response to the variation in P sw. It proved that the enhancement of P sw increases the energetic electrons fluxes, which provides free energies for the chorus amplification. Furthermore, the wave growth rates calculated using linear theory increases and the central frequency of the chorus waves shifts to a higher frequency when the P sw enhancement is greater, which are also consistent well with the observations. The results provide a direct evidence that the P sw play an important role in the long-time variation of whistler-mode chorus waves inside the magnetopause. The whistler-mode chorus waves are one of the most important plasma waves in the Earth’s magnetosphere. Generally, the amplitude of whistler-mode chorus waves prefers to strengthen when the energetic fluxes of anisotropic electrons increase outside the plasmapause. This characteristic is commonly associated with the geomagnetic storms or substorms. However, the relationship between the solar wind dynamic pressure (P sw) and the long-time variation of chorus waves during the quiet period of the geomagnetic activity still needs more detailed investigations. In this paper, based on MMS observations, we present a chorus event just observed in the inner side of magnetopause without obvious geomagnetic storms or substroms. Interestingly, during this time interval, some P sw fluctuations were recorded. Both the amplitudes and frequencies of chorus waves changed as a response to the variation in P sw. It proved that the enhancement of P sw increases the energetic electrons fluxes, which provides free energies for the chorus amplification. Furthermore, the wave growth rates calculated using linear theory increases and the central frequency of the chorus waves shifts to a higher frequency when the P sw enhancement is greater, which are also consistent well with the observations. The results provide a direct evidence that the P sw play an important role in the long-time variation of whistler-mode chorus waves inside the magnetopause. Energetic electron flux Elsevier Whistler-mode chorus waves Elsevier Wave-particle interaction Elsevier Solar wind Elsevier Li, Haimeng oth Tang, Rongxin oth Zhong, Zhihong oth Zhang, He oth Li, Qiang oth Enthalten in Elsevier Science Bargi-Souza, Paula ELSEVIER Posttranscriptional actions of triiodothyronine on 2018 including COSPAR information bulletin : the official journal of the Committee on Space Research (COSPAR), a scientific committee of the International Council of Scientific Unions (ICSU) Amsterdam [u.a.] (DE-627)ELV000905844 volume:65 year:2020 number:11 day:1 month:06 pages:2551-2558 extent:8 https://doi.org/10.1016/j.asr.2020.03.006 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA 44.89 Endokrinologie VZ AR 65 2020 11 1 0601 2551-2558 8 |
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variation of dayside chorus waves associated with solar wind dynamic pressure based on mms observations |
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Variation of dayside chorus waves associated with solar wind dynamic pressure based on MMS observations |
| abstract |
The whistler-mode chorus waves are one of the most important plasma waves in the Earth’s magnetosphere. Generally, the amplitude of whistler-mode chorus waves prefers to strengthen when the energetic fluxes of anisotropic electrons increase outside the plasmapause. This characteristic is commonly associated with the geomagnetic storms or substorms. However, the relationship between the solar wind dynamic pressure (P sw) and the long-time variation of chorus waves during the quiet period of the geomagnetic activity still needs more detailed investigations. In this paper, based on MMS observations, we present a chorus event just observed in the inner side of magnetopause without obvious geomagnetic storms or substroms. Interestingly, during this time interval, some P sw fluctuations were recorded. Both the amplitudes and frequencies of chorus waves changed as a response to the variation in P sw. It proved that the enhancement of P sw increases the energetic electrons fluxes, which provides free energies for the chorus amplification. Furthermore, the wave growth rates calculated using linear theory increases and the central frequency of the chorus waves shifts to a higher frequency when the P sw enhancement is greater, which are also consistent well with the observations. The results provide a direct evidence that the P sw play an important role in the long-time variation of whistler-mode chorus waves inside the magnetopause. |
| abstractGer |
The whistler-mode chorus waves are one of the most important plasma waves in the Earth’s magnetosphere. Generally, the amplitude of whistler-mode chorus waves prefers to strengthen when the energetic fluxes of anisotropic electrons increase outside the plasmapause. This characteristic is commonly associated with the geomagnetic storms or substorms. However, the relationship between the solar wind dynamic pressure (P sw) and the long-time variation of chorus waves during the quiet period of the geomagnetic activity still needs more detailed investigations. In this paper, based on MMS observations, we present a chorus event just observed in the inner side of magnetopause without obvious geomagnetic storms or substroms. Interestingly, during this time interval, some P sw fluctuations were recorded. Both the amplitudes and frequencies of chorus waves changed as a response to the variation in P sw. It proved that the enhancement of P sw increases the energetic electrons fluxes, which provides free energies for the chorus amplification. Furthermore, the wave growth rates calculated using linear theory increases and the central frequency of the chorus waves shifts to a higher frequency when the P sw enhancement is greater, which are also consistent well with the observations. The results provide a direct evidence that the P sw play an important role in the long-time variation of whistler-mode chorus waves inside the magnetopause. |
| abstract_unstemmed |
The whistler-mode chorus waves are one of the most important plasma waves in the Earth’s magnetosphere. Generally, the amplitude of whistler-mode chorus waves prefers to strengthen when the energetic fluxes of anisotropic electrons increase outside the plasmapause. This characteristic is commonly associated with the geomagnetic storms or substorms. However, the relationship between the solar wind dynamic pressure (P sw) and the long-time variation of chorus waves during the quiet period of the geomagnetic activity still needs more detailed investigations. In this paper, based on MMS observations, we present a chorus event just observed in the inner side of magnetopause without obvious geomagnetic storms or substroms. Interestingly, during this time interval, some P sw fluctuations were recorded. Both the amplitudes and frequencies of chorus waves changed as a response to the variation in P sw. It proved that the enhancement of P sw increases the energetic electrons fluxes, which provides free energies for the chorus amplification. Furthermore, the wave growth rates calculated using linear theory increases and the central frequency of the chorus waves shifts to a higher frequency when the P sw enhancement is greater, which are also consistent well with the observations. The results provide a direct evidence that the P sw play an important role in the long-time variation of whistler-mode chorus waves inside the magnetopause. |
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