Lower hybrid frequency range waves generated by ion polarization drift due to electromagnetic ion cyclotron waves: Analysis of an event observed by the Van Allen Probe B

G. V. Khazanov, S. Boardsen, E. N. Krivorutsky, M. J. Engebretson, D. Sibeck, S. Chen, A. Breneman

Research output: Contribution to journalArticlepeer-review

2 Scopus citations

Abstract

We analyze a wave event that occurred near noon between 07:03 and 07:08 UT on 23 February 2014 detected by the Van Allen Probes B spacecraft, where waves in the lower hybrid frequency range (LHFR) and electromagnetic ion cyclotron (EMIC) waves are observed to be highly correlated, with Pearson correlation coefficient of ~0.86. We assume that the correlation is the result of LHFR wave generation by the ions' polarization drift in the electric field of the EMIC waves. To check this assumption the drift velocities of electrons and H+, He+, and O+ ions in the measured EMIC wave electric field were modeled. Then the LHFR wave linear instantaneous growth rates for plasma with these changing drift velocities and different plasma compositions were calculated. The time distribution of these growth rates, their frequency distribution, and the frequency dependence of the ratio of the LHFR wave power spectral density (PSD) parallel and perpendicular to the ambient magnetic field to the total PSD were found. These characteristics of the growth rates were compared with the corresponding characteristics of the observed LHFR activity. Reasonable agreement between these features and the strong correlation between EMIC and LHFR energy densities support the assumption that the LHFR wave generation can be caused by the ions' polarization drift in the electric field of an EMIC wave.

Original languageEnglish (US)
Pages (from-to)449-463
Number of pages15
JournalJournal of Geophysical Research: Space Physics
Volume122
Issue number1
DOIs
StatePublished - Jan 1 2017

Bibliographical note

Funding Information:
Funding support for this study was provided by NASA the Van Allen Probes (formerly known as the Radiation Belt Storm Probes (RBSP)) Project, including NASA prime contract NAS5-01072, and NASA LWS Program. The data for this paper are available from George V. Khazanov at george.v.khazanov@nasa.gov. The EMFISIS data from the Van Allen Probes are available at http://emfisis.physics.uiowa.edu/. The Van Allen Probes EFW data are available at http://www.space.umn.edu/missions/rbspefw-home-university-of-minnesota/. OMNI data are available at the NASA/GSFC's Space Physics Data Facility's CDAWeb, at http://cdaweb.gsfc.nasa.gov/istp_public/. We acknowledge use of these data.

Publisher Copyright:
©2016. American Geophysical Union. All Rights Reserved.

Keywords

  • nonlinear phenomena
  • parametric processes
  • wave/wave interactions

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