Journal article
Fine Harmonic Structure of Equatorial Noise with a Quasiperiodic Modulation
Journal of geophysical research. Space physics, Vol.125(3), e2019JA027509
03/01/2020
DOI: 10.1029/2019JA027509
Abstract
Equatorial noise emissions (fast magnetosonic waves) are electromagnetic waves observed routinely in the equatorial region of the inner magnetosphere. They propagate with wave vectors nearly perpendicular to the ambient magnetic field; that is, they are limited to frequencies below the lower hybrid frequency. The waves are generated by instabilities of ring-like proton distribution functions, which result in their fine harmonic structure with intensity maxima close to harmonics of the proton cyclotron frequency in the source region. Although most equatorial noise emissions are continuous in time, some events exhibit a clear quasiperiodic time modulation of the wave intensity, with typical modulation periods on the order of minutes. We analyze 72 such events (17 observed by the Cluster spacecraft, 55 observed by the Van Allen Probes spacecraft) for which high-resolution data were available. The analysis of the observed harmonic structure allows us to determine source radial distances of the events. It is found that the calculated source radial distances are generally close to the radial distances where the events were observed. The harmonic numbers where the events are generated range between about 12 and 30. Two events for which the spacecraft passed through the generation region were identified and analyzed. No simultaneous ultra-low-frequency magnetic field pulsations and no periodic plasma number density variations were observed. Although the in situ measured proton distribution functions were shown to be responsible for the wave growth, an insufficient resolution of the particle instruments prevented us from detecting a quasiperiodic modulation possibly present in the particle data.
Details
- Title: Subtitle
- Fine Harmonic Structure of Equatorial Noise with a Quasiperiodic Modulation
- Creators
- F. Nemec - Charles UniversityA. Tomori - Czech Academy of Sciences, Institute of Atmospheric PhysicsO. Santolik - Czech Academy of Sciences, Institute of Atmospheric PhysicsS. A. Boardsen - University of Maryland, Baltimore CountyG. B. Hospodarsky - University of IowaW. S. Kurth - University of IowaJ. S. Pickett - Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USAC. Kletzing - University of Iowa
- Resource Type
- Journal article
- Publication Details
- Journal of geophysical research. Space physics, Vol.125(3), e2019JA027509
- DOI
- 10.1029/2019JA027509
- ISSN
- 2169-9380
- eISSN
- 2169-9402
- Publisher
- Amer Geophysical Union
- Number of pages
- 12
- Grant note
- 18-00844S / GACR; Grant Agency of the Czech Republic LTAUSA17070 / MSMT; Ministry of Education, Youth & Sports - Czech Republic 921647; NAS5-01072 / NASA through JHU/APL under NASA Praemium Academiae award from the CAS
- Language
- English
- Date published
- 03/01/2020
- Academic Unit
- Physics and Astronomy
- Record Identifier
- 9984428779802771
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