Oxygen cyclotron harmonic waves observed using Van Allen Probes
Abstract Fine structured multiple-harmonic electromagnetic emissions at frequencies around the equatorial oxygen cyclotron harmonics are observed by Van Allen Probe A outside the core plasmasphere (L~5) off the magnetic equator (MLAT~−7.5°) during a geomagnetic storm. We find that the multiple-harmo...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Yu, XiongDong [verfasserIn] Yuan, ZhiGang [verfasserIn] Wang, DeDong [verfasserIn] Huang, ShiYong [verfasserIn] Li, HaiMeng [verfasserIn] Yu, Tao [verfasserIn] Qiao, Zheng [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2017 |
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| Schlagwörter: |
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| Übergeordnetes Werk: |
Enthalten in: Science in China - Heidelberg : Springer, 1997, 60(2017), 7 vom: 12. Apr., Seite 1310-1316 |
|---|---|
| Übergeordnetes Werk: |
volume:60 ; year:2017 ; number:7 ; day:12 ; month:04 ; pages:1310-1316 |
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| DOI / URN: |
10.1007/s11430-016-9024-3 |
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| 520 | |a Abstract Fine structured multiple-harmonic electromagnetic emissions at frequencies around the equatorial oxygen cyclotron harmonics are observed by Van Allen Probe A outside the core plasmasphere (L~5) off the magnetic equator (MLAT~−7.5°) during a geomagnetic storm. We find that the multiple-harmonic emissions have power spectrum density (PSD) peaks during 2–8 equatorial oxygen gyroharmonics (f ~ n%$f_{O^{+}}%$, n=2–8), while the fundamental mode (n=1) is absent, implying that the harmonic waves are generated near the equator and propagate into the observation region. Additionally, these electromagnetic emissions are linearly polarized. Different from the equatorial noise emission that propagates considerably obliquely, these emissions have moderate wave normal angles (approximately 40°–60°), which predominately increase as the harmonic number increases. Considering their frequency and wave normal angle characteristics, it is suggested that these multiple-harmonic emissions play an important role in the dynamic variation of radiation belt electrons. | ||
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| 700 | 1 | |a Yu, Tao |e verfasserin |4 aut | |
| 700 | 1 | |a Qiao, Zheng |e verfasserin |4 aut | |
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10.1007/s11430-016-9024-3 doi (DE-627)SPR019249519 (SPR)s11430-016-9024-3-e DE-627 ger DE-627 rakwb eng 550 ASE 38.00 bkl Yu, XiongDong verfasserin aut Oxygen cyclotron harmonic waves observed using Van Allen Probes 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Fine structured multiple-harmonic electromagnetic emissions at frequencies around the equatorial oxygen cyclotron harmonics are observed by Van Allen Probe A outside the core plasmasphere (L~5) off the magnetic equator (MLAT~−7.5°) during a geomagnetic storm. We find that the multiple-harmonic emissions have power spectrum density (PSD) peaks during 2–8 equatorial oxygen gyroharmonics (f ~ n%$f_{O^{+}}%$, n=2–8), while the fundamental mode (n=1) is absent, implying that the harmonic waves are generated near the equator and propagate into the observation region. Additionally, these electromagnetic emissions are linearly polarized. Different from the equatorial noise emission that propagates considerably obliquely, these emissions have moderate wave normal angles (approximately 40°–60°), which predominately increase as the harmonic number increases. Considering their frequency and wave normal angle characteristics, it is suggested that these multiple-harmonic emissions play an important role in the dynamic variation of radiation belt electrons. Oxygen cyclotron harmonic waves (dpeaa)DE-He213 Van Allen Probes (dpeaa)DE-He213 Ring current ions (dpeaa)DE-He213 Radiation belt (dpeaa)DE-He213 Yuan, ZhiGang verfasserin aut Wang, DeDong verfasserin aut Huang, ShiYong verfasserin aut Li, HaiMeng verfasserin aut Yu, Tao verfasserin aut Qiao, Zheng verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 60(2017), 7 vom: 12. Apr., Seite 1310-1316 (DE-627)385614748 (DE-600)2142896-7 1862-2801 nnns volume:60 year:2017 number:7 day:12 month:04 pages:1310-1316 https://dx.doi.org/10.1007/s11430-016-9024-3 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-GGO SSG-OPC-ASE GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_152 GBV_ILN_161 GBV_ILN_171 GBV_ILN_187 GBV_ILN_224 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 38.00 ASE AR 60 2017 7 12 04 1310-1316 |
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10.1007/s11430-016-9024-3 doi (DE-627)SPR019249519 (SPR)s11430-016-9024-3-e DE-627 ger DE-627 rakwb eng 550 ASE 38.00 bkl Yu, XiongDong verfasserin aut Oxygen cyclotron harmonic waves observed using Van Allen Probes 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Fine structured multiple-harmonic electromagnetic emissions at frequencies around the equatorial oxygen cyclotron harmonics are observed by Van Allen Probe A outside the core plasmasphere (L~5) off the magnetic equator (MLAT~−7.5°) during a geomagnetic storm. We find that the multiple-harmonic emissions have power spectrum density (PSD) peaks during 2–8 equatorial oxygen gyroharmonics (f ~ n%$f_{O^{+}}%$, n=2–8), while the fundamental mode (n=1) is absent, implying that the harmonic waves are generated near the equator and propagate into the observation region. Additionally, these electromagnetic emissions are linearly polarized. Different from the equatorial noise emission that propagates considerably obliquely, these emissions have moderate wave normal angles (approximately 40°–60°), which predominately increase as the harmonic number increases. Considering their frequency and wave normal angle characteristics, it is suggested that these multiple-harmonic emissions play an important role in the dynamic variation of radiation belt electrons. Oxygen cyclotron harmonic waves (dpeaa)DE-He213 Van Allen Probes (dpeaa)DE-He213 Ring current ions (dpeaa)DE-He213 Radiation belt (dpeaa)DE-He213 Yuan, ZhiGang verfasserin aut Wang, DeDong verfasserin aut Huang, ShiYong verfasserin aut Li, HaiMeng verfasserin aut Yu, Tao verfasserin aut Qiao, Zheng verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 60(2017), 7 vom: 12. Apr., Seite 1310-1316 (DE-627)385614748 (DE-600)2142896-7 1862-2801 nnns volume:60 year:2017 number:7 day:12 month:04 pages:1310-1316 https://dx.doi.org/10.1007/s11430-016-9024-3 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-GGO SSG-OPC-ASE GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_152 GBV_ILN_161 GBV_ILN_171 GBV_ILN_187 GBV_ILN_224 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 38.00 ASE AR 60 2017 7 12 04 1310-1316 |
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10.1007/s11430-016-9024-3 doi (DE-627)SPR019249519 (SPR)s11430-016-9024-3-e DE-627 ger DE-627 rakwb eng 550 ASE 38.00 bkl Yu, XiongDong verfasserin aut Oxygen cyclotron harmonic waves observed using Van Allen Probes 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Fine structured multiple-harmonic electromagnetic emissions at frequencies around the equatorial oxygen cyclotron harmonics are observed by Van Allen Probe A outside the core plasmasphere (L~5) off the magnetic equator (MLAT~−7.5°) during a geomagnetic storm. We find that the multiple-harmonic emissions have power spectrum density (PSD) peaks during 2–8 equatorial oxygen gyroharmonics (f ~ n%$f_{O^{+}}%$, n=2–8), while the fundamental mode (n=1) is absent, implying that the harmonic waves are generated near the equator and propagate into the observation region. Additionally, these electromagnetic emissions are linearly polarized. Different from the equatorial noise emission that propagates considerably obliquely, these emissions have moderate wave normal angles (approximately 40°–60°), which predominately increase as the harmonic number increases. Considering their frequency and wave normal angle characteristics, it is suggested that these multiple-harmonic emissions play an important role in the dynamic variation of radiation belt electrons. Oxygen cyclotron harmonic waves (dpeaa)DE-He213 Van Allen Probes (dpeaa)DE-He213 Ring current ions (dpeaa)DE-He213 Radiation belt (dpeaa)DE-He213 Yuan, ZhiGang verfasserin aut Wang, DeDong verfasserin aut Huang, ShiYong verfasserin aut Li, HaiMeng verfasserin aut Yu, Tao verfasserin aut Qiao, Zheng verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 60(2017), 7 vom: 12. Apr., Seite 1310-1316 (DE-627)385614748 (DE-600)2142896-7 1862-2801 nnns volume:60 year:2017 number:7 day:12 month:04 pages:1310-1316 https://dx.doi.org/10.1007/s11430-016-9024-3 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-GGO SSG-OPC-ASE GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_152 GBV_ILN_161 GBV_ILN_171 GBV_ILN_187 GBV_ILN_224 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 38.00 ASE AR 60 2017 7 12 04 1310-1316 |
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10.1007/s11430-016-9024-3 doi (DE-627)SPR019249519 (SPR)s11430-016-9024-3-e DE-627 ger DE-627 rakwb eng 550 ASE 38.00 bkl Yu, XiongDong verfasserin aut Oxygen cyclotron harmonic waves observed using Van Allen Probes 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Fine structured multiple-harmonic electromagnetic emissions at frequencies around the equatorial oxygen cyclotron harmonics are observed by Van Allen Probe A outside the core plasmasphere (L~5) off the magnetic equator (MLAT~−7.5°) during a geomagnetic storm. We find that the multiple-harmonic emissions have power spectrum density (PSD) peaks during 2–8 equatorial oxygen gyroharmonics (f ~ n%$f_{O^{+}}%$, n=2–8), while the fundamental mode (n=1) is absent, implying that the harmonic waves are generated near the equator and propagate into the observation region. Additionally, these electromagnetic emissions are linearly polarized. Different from the equatorial noise emission that propagates considerably obliquely, these emissions have moderate wave normal angles (approximately 40°–60°), which predominately increase as the harmonic number increases. Considering their frequency and wave normal angle characteristics, it is suggested that these multiple-harmonic emissions play an important role in the dynamic variation of radiation belt electrons. Oxygen cyclotron harmonic waves (dpeaa)DE-He213 Van Allen Probes (dpeaa)DE-He213 Ring current ions (dpeaa)DE-He213 Radiation belt (dpeaa)DE-He213 Yuan, ZhiGang verfasserin aut Wang, DeDong verfasserin aut Huang, ShiYong verfasserin aut Li, HaiMeng verfasserin aut Yu, Tao verfasserin aut Qiao, Zheng verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 60(2017), 7 vom: 12. Apr., Seite 1310-1316 (DE-627)385614748 (DE-600)2142896-7 1862-2801 nnns volume:60 year:2017 number:7 day:12 month:04 pages:1310-1316 https://dx.doi.org/10.1007/s11430-016-9024-3 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-GGO SSG-OPC-ASE GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_152 GBV_ILN_161 GBV_ILN_171 GBV_ILN_187 GBV_ILN_224 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 38.00 ASE AR 60 2017 7 12 04 1310-1316 |
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10.1007/s11430-016-9024-3 doi (DE-627)SPR019249519 (SPR)s11430-016-9024-3-e DE-627 ger DE-627 rakwb eng 550 ASE 38.00 bkl Yu, XiongDong verfasserin aut Oxygen cyclotron harmonic waves observed using Van Allen Probes 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Fine structured multiple-harmonic electromagnetic emissions at frequencies around the equatorial oxygen cyclotron harmonics are observed by Van Allen Probe A outside the core plasmasphere (L~5) off the magnetic equator (MLAT~−7.5°) during a geomagnetic storm. We find that the multiple-harmonic emissions have power spectrum density (PSD) peaks during 2–8 equatorial oxygen gyroharmonics (f ~ n%$f_{O^{+}}%$, n=2–8), while the fundamental mode (n=1) is absent, implying that the harmonic waves are generated near the equator and propagate into the observation region. Additionally, these electromagnetic emissions are linearly polarized. Different from the equatorial noise emission that propagates considerably obliquely, these emissions have moderate wave normal angles (approximately 40°–60°), which predominately increase as the harmonic number increases. Considering their frequency and wave normal angle characteristics, it is suggested that these multiple-harmonic emissions play an important role in the dynamic variation of radiation belt electrons. Oxygen cyclotron harmonic waves (dpeaa)DE-He213 Van Allen Probes (dpeaa)DE-He213 Ring current ions (dpeaa)DE-He213 Radiation belt (dpeaa)DE-He213 Yuan, ZhiGang verfasserin aut Wang, DeDong verfasserin aut Huang, ShiYong verfasserin aut Li, HaiMeng verfasserin aut Yu, Tao verfasserin aut Qiao, Zheng verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 60(2017), 7 vom: 12. Apr., Seite 1310-1316 (DE-627)385614748 (DE-600)2142896-7 1862-2801 nnns volume:60 year:2017 number:7 day:12 month:04 pages:1310-1316 https://dx.doi.org/10.1007/s11430-016-9024-3 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-GGO SSG-OPC-ASE GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_152 GBV_ILN_161 GBV_ILN_171 GBV_ILN_187 GBV_ILN_224 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 38.00 ASE AR 60 2017 7 12 04 1310-1316 |
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We find that the multiple-harmonic emissions have power spectrum density (PSD) peaks during 2–8 equatorial oxygen gyroharmonics (f ~ n%$f_{O^{+}}%$, n=2–8), while the fundamental mode (n=1) is absent, implying that the harmonic waves are generated near the equator and propagate into the observation region. Additionally, these electromagnetic emissions are linearly polarized. Different from the equatorial noise emission that propagates considerably obliquely, these emissions have moderate wave normal angles (approximately 40°–60°), which predominately increase as the harmonic number increases. 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Oxygen cyclotron harmonic waves observed using Van Allen Probes |
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Abstract Fine structured multiple-harmonic electromagnetic emissions at frequencies around the equatorial oxygen cyclotron harmonics are observed by Van Allen Probe A outside the core plasmasphere (L~5) off the magnetic equator (MLAT~−7.5°) during a geomagnetic storm. We find that the multiple-harmonic emissions have power spectrum density (PSD) peaks during 2–8 equatorial oxygen gyroharmonics (f ~ n%$f_{O^{+}}%$, n=2–8), while the fundamental mode (n=1) is absent, implying that the harmonic waves are generated near the equator and propagate into the observation region. Additionally, these electromagnetic emissions are linearly polarized. Different from the equatorial noise emission that propagates considerably obliquely, these emissions have moderate wave normal angles (approximately 40°–60°), which predominately increase as the harmonic number increases. Considering their frequency and wave normal angle characteristics, it is suggested that these multiple-harmonic emissions play an important role in the dynamic variation of radiation belt electrons. |
| abstractGer |
Abstract Fine structured multiple-harmonic electromagnetic emissions at frequencies around the equatorial oxygen cyclotron harmonics are observed by Van Allen Probe A outside the core plasmasphere (L~5) off the magnetic equator (MLAT~−7.5°) during a geomagnetic storm. We find that the multiple-harmonic emissions have power spectrum density (PSD) peaks during 2–8 equatorial oxygen gyroharmonics (f ~ n%$f_{O^{+}}%$, n=2–8), while the fundamental mode (n=1) is absent, implying that the harmonic waves are generated near the equator and propagate into the observation region. Additionally, these electromagnetic emissions are linearly polarized. Different from the equatorial noise emission that propagates considerably obliquely, these emissions have moderate wave normal angles (approximately 40°–60°), which predominately increase as the harmonic number increases. Considering their frequency and wave normal angle characteristics, it is suggested that these multiple-harmonic emissions play an important role in the dynamic variation of radiation belt electrons. |
| abstract_unstemmed |
Abstract Fine structured multiple-harmonic electromagnetic emissions at frequencies around the equatorial oxygen cyclotron harmonics are observed by Van Allen Probe A outside the core plasmasphere (L~5) off the magnetic equator (MLAT~−7.5°) during a geomagnetic storm. We find that the multiple-harmonic emissions have power spectrum density (PSD) peaks during 2–8 equatorial oxygen gyroharmonics (f ~ n%$f_{O^{+}}%$, n=2–8), while the fundamental mode (n=1) is absent, implying that the harmonic waves are generated near the equator and propagate into the observation region. Additionally, these electromagnetic emissions are linearly polarized. Different from the equatorial noise emission that propagates considerably obliquely, these emissions have moderate wave normal angles (approximately 40°–60°), which predominately increase as the harmonic number increases. Considering their frequency and wave normal angle characteristics, it is suggested that these multiple-harmonic emissions play an important role in the dynamic variation of radiation belt electrons. |
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We find that the multiple-harmonic emissions have power spectrum density (PSD) peaks during 2–8 equatorial oxygen gyroharmonics (f ~ n%$f_{O^{+}}%$, n=2–8), while the fundamental mode (n=1) is absent, implying that the harmonic waves are generated near the equator and propagate into the observation region. Additionally, these electromagnetic emissions are linearly polarized. Different from the equatorial noise emission that propagates considerably obliquely, these emissions have moderate wave normal angles (approximately 40°–60°), which predominately increase as the harmonic number increases. 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