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Hydromagnetic eigen-oscillations in the dipolar field
https://nipr.repo.nii.ac.jp/records/1410
https://nipr.repo.nii.ac.jp/records/1410f529a2f2-1306-4fe2-a8c7-5eea1852e96b
名前 / ファイル | ライセンス | アクション |
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KJ00000012044 (3.8 MB)
|
Item type | 紀要論文(ELS) / Departmental Bulletin Paper(1) | |||||
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公開日 | 1983-03-01 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | Hydromagnetic eigen-oscillations in the dipolar field | |||||
言語 | ||||||
言語 | eng | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_6501 | |||||
資源タイプ | departmental bulletin paper | |||||
ページ属性 | ||||||
内容記述タイプ | Other | |||||
内容記述 | P(論文) | |||||
著者名(英) |
Yumoto, Kiyohumi
× Yumoto, Kiyohumi× Eitoku, Akito× Saito, Takao |
|||||
著者所属(英) | ||||||
en | ||||||
Onagawa Magnetic Observatory and Geophysical Institute, Tohoku University | ||||||
著者所属(英) | ||||||
en | ||||||
Onagawa Magnetic Observatory and Geophysical Institute,Tohoku University | ||||||
著者所属(英) | ||||||
en | ||||||
Onagawa Magnetic Observatory and Geophysical Institute,Tohoku University | ||||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | MHD equations in the dipolar coordinates are analyzed for an idealized model in which the earth surface is assumed to be a perfect conductor. For the case of standing resonance waves, i. e., the guided toroidal and the guided poloidal waves, the eigenperiods are determined mainly by the mass density near the equatorial plane in the magnetosphere. The eigenperiods of the standing waves importantly depend on the mass density of the heavy ions outside the plasmapause. The resonance oscillations are expected to occur only on a field line having L-values within a narrow range, since a displacement of MHD fluid in the equatorial plane is of the order of 0.1 R_E for a perturbed electric field ∿2mV/m near L=10. The relation of the electric field wave amplitude (δE) of the standing oscillation to the displacement ((δξ)_<eq>) is represented by |δE|=B_0(L)^<-3>・(δξ)_<eq> near the magnetic equator. The magnetic perturbation fields of the standing oscillations in the equatorial plane are one order smaller than those in the ionosphere for a case of perfect reflection. The conditions of the coupling oscillations of an Alfven wave and a compressional wave are theoretically discussed for the special case of highly asymmetric modes. | |||||
雑誌書誌ID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AA00733561 | |||||
書誌情報 |
Memoirs of National Institute of Polar Research. Special issue 巻 26, p. 61-80, 発行日 1983-03 |