Occurrence of EMIC waves and plasmaspheric plasmas derived from THEMIS observations in the outer magnetosphere: Revisit
DC Field | Value | Language |
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dc.contributor.author | Kim, Gi-Jeong | - |
dc.contributor.author | Kim, Khan-Hyuk | - |
dc.contributor.author | Lee, Dong-Hun | - |
dc.contributor.author | Kwan, Hyuckjin | - |
dc.contributor.author | Park, Jong-Sun | - |
dc.date.accessioned | 2017-08-03T12:51:05Z | - |
dc.date.available | 2017-08-03T12:51:05Z | - |
dc.date.issued | 2016 | - |
dc.description.abstract | We have statistically studied the relationship between electromagnetic ion cyclotron (EMIC) waves and cold plasmaspheric plasma (Nsp) in the L range of 6-12 using the Time History of Events and Macroscale Interactions during Substorms (THEMIS) data for 2008-2011. The important observational results are as follows: (1) Under quiet geomagnetic conditions (Kp≤ 1), the maximum occurrence rate of the hydrogen (H) band EMIC waves appears in the early morning sector (0600-0900 MLT) at the outermost region (L = 10-12). (2) Under moderate and disturbed conditions (Kp≥ 2), the H-band occurrence rate is higher in the morning-to-early afternoon sector for L> 10. (3) The high occurrence region of helium (He) band waves for Kp≤ 1 varies from L = 7 to 12 in radial distances along the local time (i.e., at L∼ 7 near noon and at L = 8-12 near late afternoon). (4) The He-band waves for Kp≥ 2 are mainly localized between 1200 and 1800 MLT with a peak around 1500-1600 MLT at L = 8-10. (5) Nsp is much higher for the He-band intervals than for the H-band intervals by a factor of 10 or more. The He-band high occurrence appears at a steep Nsp gradient region. (6) The morning-afternoon asymmetry of the normalized frequency seen both in H-band and He-band is similar to the asymmetric distribution of Nsp along the local time. These observations indicate that the cold plasma density plays a significant role in determining the spectral properties of EMIC waves. We discuss whether a morning-afternoon asymmetry of the EMIC wave properties can be explained by the spatial distribution of cold plasmaspheric plasma. | - |
dc.language | English | - |
dc.subject | Astronomy & Astrophysics | - |
dc.title | Occurrence of EMIC waves and plasmaspheric plasmas derived from THEMIS observations in the outer magnetosphere: Revisit | - |
dc.type | Article | - |
dc.identifier.bibliographicCitation | Kim, Gi-Jeong, et al. 2016. "Occurrence of EMIC waves and plasmaspheric plasmas derived from THEMIS observations in the outer magnetosphere: Revisit". <em>Journal of Geophysical Research: Space Physics</em>, 121(10): 9443-9458. | - |
dc.citation.title | Journal of Geophysical Research: Space Physics | - |
dc.citation.volume | 121 | - |
dc.citation.number | 10 | - |
dc.citation.page | 9443-9458 | - |
dc.identifier.doi | 10.1002/2016JA023108 | - |
dc.subject.keyword | EMIC waves | - |
dc.identifier.scopusid | 2-s2.0-84991111482 | - |
dc.identifier.wosid | 000388965900010 | - |
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