GSTDTAP  > 气候变化
DOI10.1029/2018GL080109
Spatial Distribution of Fine-Structured and Unstructured EMIC Waves Observed by The Arase Satellite
Matsuda, S.1; Kasahara, Y.2; Miyoshi, Y.3; Nomura, R.4; Shoji, M.3; Matsuoka, A.1; Kasaba, Y.5; Kurita, S.3; Teramoto, M.3; Ishisaka, K.6
2018-11-16
发表期刊GEOPHYSICAL RESEARCH LETTERS
ISSN0094-8276
EISSN1944-8007
出版年2018
卷号45期号:21页码:11530-11538
文章类型Article
语种英语
国家Japan
英文摘要

We surveyed 378 electromagnetic ion cyclotron (EMIC) wave events using Arase during the first 12 months. We discriminated the observed EMIC waves into two types (fine-structured EMIC waves and unstructured EMIC waves), according to whether or not they exhibited clear periodic amplitude modulations. We found a clear afternoon peak in the occurrence probability of unstructured EMIC waves in the region of L = 5-9. Fine-structured EMIC waves were mainly distributed in the off-equatorial region, and their occurrence probability was clearly high around the noon sector. Such noon sector EMIC wave peaks had not been found in the THEMIS, AMPTE, or Cluster measurements, due to their limited L shell coverages. The Van Allen probes, too, were not able to measure the major region of fine-structured EMIC waves because of their limited latitudinal coverage. Our unique statistical results demonstrate the importance of discriminating the wave structures as well as of performing observations over a wide range of latitudes.


Plain Language Summary The spatial distribution of electromagnetic ion cyclotron (EMIC) waves is important and fundamental information from the point of view of wave-particle interaction process. Several studies have determined the distributions of EMIC waves. However, they have been controversial, because there are several possible mechanisms for generating EMIC waves. We discriminated 378 events observed by Arase into two types, according to whether or not they exhibited clear periodic amplitude modulations. We found a clear afternoon peak in the occurrence probability of unstructured EMIC waves in the region of L = 5-9. This is consistent with previous observations. Fine-structured EMIC waves were mainly distributed in the off-equatorial region, and their occurrence probability was clearly high around noon. Such noon peaks had not been found in the THEMIS, AMPTE, or Cluster measurements, due to their limited L shell coverages. The Van Allen probes measured the region of L = 2-6, but they also did not report such a noon sector peak. Our statistical results suggest that the Van Allen probes, too, were not able to measure the major region of fine-structured EMIC waves because of their limited latitudinal coverage. Our unique statistical results demonstrate the importance of discriminating the wave structures as well as of performing observations over a wide range of latitudes.


领域气候变化
收录类别SCI-E
WOS记录号WOS:000451832600003
WOS关键词RESONANT SCATTERING ; PULSATIONS ; AKEBONO ; MAGNETOSPHERE ; EMISSIONS ; PLASMA
WOS类目Geosciences, Multidisciplinary
WOS研究方向Geology
引用统计
文献类型期刊论文
条目标识符http://119.78.100.173/C666/handle/2XK7JSWQ/25916
专题气候变化
作者单位1.Japan Aerosp Explorat Agcy, Inst Space & Astronaut Sci, Sagamihara, Kanagawa, Japan;
2.Kanazawa Univ, Grad Sch Nat Sci & Technol, Kanazawa, Ishikawa, Japan;
3.Nagoya Univ, Inst Space Earth Environm Res, Nagoya, Aichi, Japan;
4.Natl Astron Observ Japan, Tokyo, Japan;
5.Tohoku Univ, Grad Sch Sci, Sendai, Miyagi, Japan;
6.Toyama Prefectural Univ, Dept Informat Syst & Syst Engn, Imizu, Toyama, Japan
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GB/T 7714
Matsuda, S.,Kasahara, Y.,Miyoshi, Y.,et al. Spatial Distribution of Fine-Structured and Unstructured EMIC Waves Observed by The Arase Satellite[J]. GEOPHYSICAL RESEARCH LETTERS,2018,45(21):11530-11538.
APA Matsuda, S..,Kasahara, Y..,Miyoshi, Y..,Nomura, R..,Shoji, M..,...&Ishisaka, K..(2018).Spatial Distribution of Fine-Structured and Unstructured EMIC Waves Observed by The Arase Satellite.GEOPHYSICAL RESEARCH LETTERS,45(21),11530-11538.
MLA Matsuda, S.,et al."Spatial Distribution of Fine-Structured and Unstructured EMIC Waves Observed by The Arase Satellite".GEOPHYSICAL RESEARCH LETTERS 45.21(2018):11530-11538.
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