Waves in the proton cyclotron frequency range in the CME observed by wind on August 7-8,1996: Theory and data
As first discussed by Farrugia et al. (J. Geophys. Res., 103, 6543, 1998), coronal mass ejections (CMEs) may support the excitation of electromagnetic ion cyclotron waves (EICWs). The proton plasma beta, and the electron temperature and anisotropy in the front region (~5 hours, translating to ~6×106...
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todo:paper_02731177_v28_n5_p747_Dasso2023-10-03T15:15:30Z Waves in the proton cyclotron frequency range in the CME observed by wind on August 7-8,1996: Theory and data Dasso, S. Farrugia, C.J. Gratton, F.T. Lepping, R.P. Ogilvie, K.W. Fitzenreiter, R.J. Anisotropy Space research Spacecraft Wind Electron temperature Electromagnetic waves magnetosphere plasma As first discussed by Farrugia et al. (J. Geophys. Res., 103, 6543, 1998), coronal mass ejections (CMEs) may support the excitation of electromagnetic ion cyclotron waves (EICWs). The proton plasma beta, and the electron temperature and anisotropy in the front region (~5 hours, translating to ~6×106 km) of the CME observed by WIND on August 7-8, 1996 favor this possible excitation. Supplementing these measured parameters by other data taken from a survey of CME properties observed by the ISEE 3 spacecraft (Gosling et al., J. Geophys. Res., 92, 8519, 1987), we solve the EICW dispersion relation numerically. We find short e-folding times of EICWs, of the order of 5 min, i.e., much less than the typical evolution time of these ejecta. We suggest that high resolution data will show enhanced power in the 0.5 Hz range. © 2001 COSPAR. Published by Elsevier Science Ltd. All rights reserved. Fil:Dasso, S. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. Fil:Gratton, F.T. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_02731177_v28_n5_p747_Dasso |
institution |
Universidad de Buenos Aires |
institution_str |
I-28 |
repository_str |
R-134 |
collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
topic |
Anisotropy Space research Spacecraft Wind Electron temperature Electromagnetic waves magnetosphere plasma |
spellingShingle |
Anisotropy Space research Spacecraft Wind Electron temperature Electromagnetic waves magnetosphere plasma Dasso, S. Farrugia, C.J. Gratton, F.T. Lepping, R.P. Ogilvie, K.W. Fitzenreiter, R.J. Waves in the proton cyclotron frequency range in the CME observed by wind on August 7-8,1996: Theory and data |
topic_facet |
Anisotropy Space research Spacecraft Wind Electron temperature Electromagnetic waves magnetosphere plasma |
description |
As first discussed by Farrugia et al. (J. Geophys. Res., 103, 6543, 1998), coronal mass ejections (CMEs) may support the excitation of electromagnetic ion cyclotron waves (EICWs). The proton plasma beta, and the electron temperature and anisotropy in the front region (~5 hours, translating to ~6×106 km) of the CME observed by WIND on August 7-8, 1996 favor this possible excitation. Supplementing these measured parameters by other data taken from a survey of CME properties observed by the ISEE 3 spacecraft (Gosling et al., J. Geophys. Res., 92, 8519, 1987), we solve the EICW dispersion relation numerically. We find short e-folding times of EICWs, of the order of 5 min, i.e., much less than the typical evolution time of these ejecta. We suggest that high resolution data will show enhanced power in the 0.5 Hz range. © 2001 COSPAR. Published by Elsevier Science Ltd. All rights reserved. |
format |
JOUR |
author |
Dasso, S. Farrugia, C.J. Gratton, F.T. Lepping, R.P. Ogilvie, K.W. Fitzenreiter, R.J. |
author_facet |
Dasso, S. Farrugia, C.J. Gratton, F.T. Lepping, R.P. Ogilvie, K.W. Fitzenreiter, R.J. |
author_sort |
Dasso, S. |
title |
Waves in the proton cyclotron frequency range in the CME observed by wind on August 7-8,1996: Theory and data |
title_short |
Waves in the proton cyclotron frequency range in the CME observed by wind on August 7-8,1996: Theory and data |
title_full |
Waves in the proton cyclotron frequency range in the CME observed by wind on August 7-8,1996: Theory and data |
title_fullStr |
Waves in the proton cyclotron frequency range in the CME observed by wind on August 7-8,1996: Theory and data |
title_full_unstemmed |
Waves in the proton cyclotron frequency range in the CME observed by wind on August 7-8,1996: Theory and data |
title_sort |
waves in the proton cyclotron frequency range in the cme observed by wind on august 7-8,1996: theory and data |
url |
http://hdl.handle.net/20.500.12110/paper_02731177_v28_n5_p747_Dasso |
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