書誌事項
- 公開日
- 1992-10
- 権利情報
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- https://www.elsevier.com/tdm/userlicense/1.0/
- DOI
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- 10.1016/0032-0633(92)90089-7
- 公開者
- Elsevier BV
この論文をさがす
説明
Abstract A review of mid-latitude and plasmaspheric hiss-type emissions observed on ground-based stations and in the Earth's magnetosphere is presented. Different approaches to modelling of these emissions are discussed. It is pointed out that mid-latitude hiss emissions are most likely to be generated in the equatorial magnetosphere where the energy of electrons is transferred to wave energy via the electron cyclotron instability. Some quantitative characteristics of these emissions are explained in terms of a quasilinear model of this instability. Many properties of plasmaspheric hiss emissions are likely to be related to the same electron cyclotron instability, although the contribution of other mechanisms cannot be excluded.
収録刊行物
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- Planetary and Space Science
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Planetary and Space Science 40 (10), 1325-1338, 1992-10
Elsevier BV
