Full Particle Simulation of Whistler‐Mode Triggered Falling‐Tone Emissions in the Magnetosphere
-
- Takeshi Nogi
- Research Institute for Sustainable Humanosphere Kyoto University Kyoto Japan
-
- Satoko Nakamura
- Research Institute for Sustainable Humanosphere Kyoto University Kyoto Japan
-
- Yoshiharu Omura
- Research Institute for Sustainable Humanosphere Kyoto University Kyoto Japan
書誌事項
- 公開日
- 2020-10
- 権利情報
-
- http://creativecommons.org/licenses/by/4.0/
- DOI
-
- 10.1029/2020ja027953
- 公開者
- American Geophysical Union (AGU)
この論文をさがす
説明
<jats:title>Abstract</jats:title><jats:p>We perform a one‐dimensional electromagnetic full particle simulation for triggered falling‐tone emissions in the Earth's magnetosphere. The equatorial region of the magnetosphere is modeled with a parabolic magnetic field approximation. The short whistler‐mode waves with a large amplitude are excited and propagate poleward from an artificial current oscillating with a constant frequency and amplitude. Following the excited waves, clear emissions are triggered with a falling frequency. Without the inhomogeneity of the background magnetic field, no triggered emission appears. The falling tone has several subpackets of amplitude and decreases the frequency in a stepwise manner. The positive resonant current formed by resonant electrons in the direction of the wave magnetic field clearly shows that an electron hill is formed in the phase space and causes the frequency decrease. The entrapping of the resonant electrons at the front of the packets and the decrease of the amplitude at the end of packets are essential for the generation of falling‐tone emissions. Each wavefront of the emission has a strongly negative resonant current <jats:styled-content>−<jats:italic>J</jats:italic><jats:sub><jats:italic>E</jats:italic></jats:sub></jats:styled-content>, which results in the wave growth. In the formation process of the resonant currents, we investigate the inhomogeneous factor <jats:italic>S</jats:italic>, which controls the nonlinear motion of the resonant electrons interacting with waves. The factor <jats:italic>S</jats:italic> consists of two terms, a frequency sweep rate and a gradient of the background magnetic field. The resonant current <jats:styled-content><jats:italic>J</jats:italic><jats:sub><jats:italic>E</jats:italic></jats:sub></jats:styled-content> in the wave packet changes its sign from negative to positive as the packet moves away from the equator, terminating the wave growth.</jats:p>
収録刊行物
-
- Journal of Geophysical Research: Space Physics
-
Journal of Geophysical Research: Space Physics 125 (10), e2020JA027953-, 2020-10
American Geophysical Union (AGU)
- Tweet
詳細情報 詳細情報について
-
- CRID
- 1360294646542586752
-
- ISSN
- 21699402
- 21699380
-
- HANDLE
- 2433/260706
-
- データソース種別
-
- Crossref
- OpenAIRE
