L
L. Y. Li
Researcher at Beihang University
Publications - 29
Citations - 614
L. Y. Li is an academic researcher from Beihang University. The author has contributed to research in topics: Van Allen radiation belt & Solar wind. The author has an hindex of 11, co-authored 26 publications receiving 417 citations. Previous affiliations of L. Y. Li include Space Science Institute.
Papers
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Journal ArticleDOI
Multiple loss processes of relativistic electrons outside the heart of outer radiation belt during a storm sudden commencement
J. Yu,L. Y. Li,J. B. Cao,Zhigang Yuan,Geoffrey D. Reeves,Daniel N. Baker,J. B. Blake,Harlan E. Spence +7 more
TL;DR: In this paper, the relativistic electron loss mainly occurs in the field-aligned direction (pitch angle α, 150°), and the flux decay of the fieldaligned electrons is independent of the spatial location variations of the two satellites.
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Roles of whistler mode waves and magnetosonic waves in changing the outer radiation belt and the slot region
L. Y. Li,J. Yu,J. B. Cao,Junying Yang,Xinlin Li,Daniel N. Baker,Geoffrey D. Reeves,Harlan E. Spence +7 more
TL;DR: In this article, the combined or competing effects of whistler-mode waves (chorus or hiss) and magnetosonic (MS) waves on energetic (0.5 ǫ) electrons inside and outside the plasmasphere were examined.
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Propagation characteristics of plasmaspheric hiss: Van Allen Probe observations and global empirical models
TL;DR: Based on the Van Allen Probe A observations from 1 October 2012 to 31 December 2014, this paper developed two empirical models to respectively describe the hiss wave normal angle (WNA) and amplitude variations in the Earth's plasmasphere for different substorm activities.
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Joint responses of geosynchronous magnetic field and relativistic electrons to external changes in solar wind dynamic pressure and interplanetary magnetic field
TL;DR: In this paper, the authors studied statistically the joint responses of magnetic field and relativistic electrons at geosynchronous orbit to interplanetary perturbations during 6 years from 2003 to 2008.
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Compression-amplified EMIC waves and their effects on relativistic electrons
TL;DR: In this paper, the periodic emissions of electromagnetic ion cyclotron (EMIC) waves near the nightside geosynchronous orbit (6.6RE) were observed during enhancement of solar wind dynamic pressure, and the relativistic electron precipitation was observed by POES satellite near the foot point (∼850 km) of the wave emission region.