KOPRI Repository

EMIC waves observed at geosynchronous orbit under quiet geomagnetic conditions (Kp ≤ 1)

Cited 12 time in scopus
Metadata Downloads
Title
EMIC waves observed at geosynchronous orbit under quiet geomagnetic conditions (Kp ≤ 1)
Other Titles
Kp≤1 조건하에서 정지궤도위성에서 관측된 EMIC 파동
Authors
Park, Jong-Sun
Jee, Geonhwa
Jin, Ho
Kwan, Hyuckjin
Lee, Ensang
Lee, Dong-Hun Lee, Dong-Hun
K. Shiokawa
Kim, Khan-Hyuk
Keywords
EMIC wave; 극지고층대기; 자기권
Issue Date
2016
Citation
Park, Jong-Sun, et al. 2016. "EMIC waves observed at geosynchronous orbit under quiet geomagnetic conditions (Kp ≤ 1)". JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 121: 1377-1390.
Abstract
We statistically study the local time distribution of the helium band electromagnetic ion cyclotron (EMIC) waves observed at geosyn- chronous orbit when geomagnetic activity was low (Kp ≤ 1). In order to iden- tify the geosynchronous EMIC waves, we use high-time resolution magnetic field data acquired from GOES 10, 11, and 12 over a two-year period from 2007 and 2008 and examine the local time distribution of EMIC events. Un- like previous studies, which reported high EMIC occurrence in the postnoon sector with a peak around 1500-1600 magnetic local time (MLT) during mag- netically disturbed times (i.e., storm and/or substorm), we observed that quiet- time EMIC waves mostly occur in a region from morning (∼0600 MLT) to afternoon (∼1600 MLT) with a peak around 1100-1200 MLT. To investigate whether the quiet-time EMIC wave occurrence has a causal relationship with magnetospheric convection enhancement or solar wind dynamic pressure vari- ations, we performed a superposed epoch analysis of solar wind parameters (solar wind speed, density, dynamic pressure, and IMF Bz) and geomagnetic indices (AE and SY M ?H). From the epoch analysis we found that solar wind dynamic pressure variation is more important parameter than AE and SY M ? H for quiet-time EMIC wave occurrence.
URI
http://repository.kopri.re.kr/handle/201206/7446
DOI
http://dx.doi.org/10.1002/2015JA021968
Files in This Item
General Conditions
      ROMEO Green
    Can archive pre-print and post-print or publisher's version/PDF
      ROMEO Blue
    Can archive post-print (ie final draft post-refereeing) or publisher's version/PDF
      ROMEO Yellow
    Can archive pre-print (ie pre-refereeing)
      ROMEO White
    Archiving not formally supported

    qrcode

    Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.

    Browse