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Gang Li

Researcher at Chinese Academy of Sciences

Publications -  459
Citations -  9506

Gang Li is an academic researcher from Chinese Academy of Sciences. The author has contributed to research in topics: Solar wind & Particle acceleration. The author has an hindex of 48, co-authored 406 publications receiving 7713 citations. Previous affiliations of Gang Li include Nanjing University of Information Science and Technology & University of California, Berkeley.

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Evidence of the solar EUV hot channel as a magnetic flux rope from remote-sensing and in-situ observations

TL;DR: In this paper, an erupting hot channel (HC) was observed prior to and during a coronal mass ejection (CME) by the Atmospheric Imaging Assembly high-temperature images, which is consistent with the high temperature and high density of the HC and support that the ejecta is the erupted HC.
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Solar cycle abundance variations in corotating interaction regions: evidence for a suprathermal ion seed population

TL;DR: In this paper, the authors surveyed the heavy ion composition of corotating interaction regions (CIRs) over the recent solar minimum and combined this with an earlier survey to cover the 1998-2011 period encompassing a full solar cycle and onset of the new cycle.
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Microwave Imaging of a Hot Flux Rope Structure during the Pre-impulsive Stage of an Eruptive M7.7 Solar Flare

TL;DR: In this paper, the authors presented the first microwave imaging study of a hot flux rope structure during the pre-impulsive stage of an eruptive M7.7 solar flare, with the Nobeyama Radioheliograph at 17 GHz.
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Spectral Properties of Large Gradual Solar Energetic Particle Events. I. Fe, O, and Seed Material

TL;DR: In this article, a survey of the SEP spectra of 46 isolated, large gradual SEP events observed at ACE during solar cycles 23 and 24 was conducted, and the authors concluded that SEP spectral properties result from many complex and competing effects, namely Q/M-dependent scattering, shock properties and the origin of the seed populations, all of which must be taken into account to develop a comprehensive picture of CME-driven shock acceleration.