- Title
- Effect of spatial density variation and O+ concentration on the growth and evolution of electromagnetic ion cyclotron waves
- Creator
- Denton, R. E.; Jordanova, V. K.; Fraser, B. J.
- Relation
- ARC.DP0772504
- Relation
- Journal of Geophysical Research: Space Physics Vol. 119, Issue 10, p. 8372-8395
- Publisher Link
- http://dx.doi.org/10.1002/2014JA020384
- Publisher
- Wiley-Blackwell Publishing
- Resource Type
- journal article
- Date
- 2014
- Description
- We simulate electromagnetic ion cyclotron (EMIC) wave growth and evolution within three regions, the plasmasphere (or plasmaspheric plume), the plasmapause, and the low-density plasmatrough outside the plasmapause. First, we use a ring current simulation with a plasmasphere model to model the particle populations that give rise to the instability for conditions observed on 9 June 2001. Then, using two different models for the cold ion composition, we do a full-scale hybrid code simulation in dipole coordinates of the EMIC waves on a meridional plane at magnetic local time = 18 and at 1900 UT within a range of L shell from L=4.9 to 6.7. EMIC waves were observed during 9 June 2001 by Geostationary Operational Environmental Satellite (GOES) spacecraft. While an exact comparison between observed and simulated spectra is not possible here, we do find significant similarities between the two, at least at one location within the region of largest wave growth. We find that the plasmapause is not a preferred region for EMIC wave growth, though waves can grow in that region. The density gradient within the plasmapause does, however, affect the orientation of wavefronts and wave vector both within the plasmapause and in adjacent regions. There is a preference for EMIC waves to be driven in the He+ band (frequencies between the O+ and He+ gyrofrequencies) within the plasmasphere, although they can also grow in the plasmatrough. If present, H+ band waves are more likely to grow in the plasmatrough. This fact, plus L dependence of the frequency and possible time evolution toward lower frequency waves, can be explained by a simple model. Large O+ concentration limits the frequency range of or even totally quenches EMIC waves. This is more likely to occur in the plasmatrough at solar maximum. Such large O+ concentration significantly affects the H+ cutoff frequency and hence the width in frequency of the stop band above the He+ gyrofrequency. EMIC wave surfaces predicted by cold plasma theory are altered by the finite temperature of the ring current H+.
- Subject
- cold density; EMIC waves; composition; O+ concentration
- Identifier
- http://hdl.handle.net/1959.13/1299390
- Identifier
- uon:19868
- Identifier
- ISSN:2169-9380
- Language
- eng
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