A statistical study of EMIC waves observed by Cluster. 1. Wave properties. EMIC Wave Properties

Allen, R. C.; Zhang, J. -C.; Kistler, L. M.; Spence, H. E.; Lin, R. -L.; Klecker, B.; Dunlop, M. W.; André, M.; Jordanova, V. K.

doi:10.1002/2015JA021333

Title: A statistical study of EMIC waves observed by Cluster. 1. Wave properties. EMIC Wave Properties

Journal Article · Thu Jul 23 00:00:00 EDT 2015 · Journal of Geophysical Research. Space Physics

DOI:https://doi.org/10.1002/2015JA021333· OSTI ID:1215508

^[1]; Zhang, J. -C. ^[2]; Kistler, L. M. ^[2]; Spence, H. E. ^[2]; Lin, R. -L. ^[3]; Klecker, B. ^[4]; Dunlop, M. W. ^[5]; André, M. ^[6]; Jordanova, V. K. ^[7]

Univ. of New Hampshire, Durham, NH (United States); Southwest Research Inst. (SwRI), San Antonio, TX (United States); Univ. of Texas, San Antonio, TX (United States)
Univ. of New Hampshire, Durham, NH (United States)
Chinese Academy of Sciences, Beijing (China)
Max-Plank-Inst. for Extraterrestrial Physics, Garching (Germany)
Rutherford Appleton Lab., Oxfordshire (United Kingdom)
Swedish Institute of Space Physics (IRF), Uppsala (Sweden)
Los Alamos National Lab. (LANL), Los Alamos, NM (United States)

Electromagnetic ion cyclotron (EMIC) waves are an important mechanism for particle energization and losses inside the magnetosphere. In order to better understand the effects of these waves on particle dynamics, detailed information about the occurrence rate, wave power, ellipticity, normal angle, energy propagation angle distributions, and local plasma parameters are required. Previous statistical studies have used in situ observations to investigate the distribution of these parameters in the magnetic local time versus L-shell (MLT-L) frame within a limited magnetic latitude (MLAT) range. In our study, we present a statistical analysis of EMIC wave properties using 10 years (2001–2010) of data from Cluster, totaling 25,431 min of wave activity. Due to the polar orbit of Cluster, we are able to investigate EMIC waves at all MLATs and MLTs. This allows us to further investigate the MLAT dependence of various wave properties inside different MLT sectors and further explore the effects of Shabansky orbits on EMIC wave generation and propagation. Thus, the statistical analysis is presented in two papers. OUr paper focuses on the wave occurrence distribution as well as the distribution of wave properties. The companion paper focuses on local plasma parameters during wave observations as well as wave generation proxies.

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Research Organization:: Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)

Sponsoring Organization:: USDOE

Grant/Contract Number:: NNX11AO82G; NNX11AB65G; 967399; AC52-06NA25396

OSTI ID:: 1215508

Report Number(s):: LA-UR-14-25307

Journal Information:: Journal of Geophysical Research. Space Physics, Vol. 120, Issue 7; ISSN 2169-9380

Publisher:: American Geophysical UnionCopyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 129 works

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