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Bo Li
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Prof. Dr. Bo Li

School of Space Science and Physics

Shandong University atWeihai, Weihai,Shandong, China 264209

Tel:0086-631-5673527

Email:bbl@sdu.edu.cn

Research Interests

Bo Li's research interests are with the roles ofhydromagneticwaves in heating the solar corona and accelerating the solar wind. He combines multi-fluid models of the solar corona and solar wind with a forward modeling approach to infer what influences the behavior of coronal plasma species in general, and those emitting Ultraviolet lines in particular.

Honors, Awards and Accomplishments

Member of the International Space Science Institute (ISSI) international team of “Slow solar wind sources and acceleration mechanisms in the corona” (2014-2015)

Professional Services

Reviewer for the Astrophysical Journal, Journal of Geophysical Research, ASP conf. proceedings, Science in China, among others.

Life member of the American Geophysical Union (AGU)

Employment History

2009.06–

Professor ofPhysics (SupportedbytheQiluYoungScholarProgram), Shandong University,China

2002.07– 2009.03

(Post-Doctoral)Research Assistant

AberystwythUniversity,UK

Education

1996.09– 2001.12

Ph.D.inSpacePhysics

UniversityofScienceandTechnology ofChina (USTC), Hefei, China

1992.09– 1996.07

B.Sc. inNuclearPhysics,USTC, Hefei, China

List of Publications (always up to date)

http://adsabs.harvard.edu/cgi-bin/nph-abs_connect?library&libname=MyPub&libid=46fa5538e5

Selected Publications

O. W. Roberts, X. Li, &B. Li, Kinetic plasma turbulence in the fast solar wind measured by Cluster,Astrophysical Journal(ApJ), 769, 58, (2013)

B. Li, S. R.Habbal, & Y.-J. Chen, The period ratio for standing kink and sausage modes in solar structures with siphon flow. I. magnetized slabs,ApJ, 767, 169 (2013)

B. Li, L.-D. Xia, & Y. Chen, Solar winds along curved magnetic field lines, Astronomy & Astrophysics (A&A), 529, A148 (2011)

Y. Chen, S.Feng,B. Li, et al., A Coronal Seismological Study with Streamer Waves,ApJ, 728, 147 (2011)

Bo Li, & Xing Li, Angular momentum transport in amulticomponentsolar wind with differentially flowing, thermally anisotropic ions, A&A, 494(1), 361-371 (2009)

Bo Li, & Xing Li, Effects of non-WKB Alfven waves on amulticomponentsolar wind with differential ion flow,ApJ, 682(1), 667-678 (2008)

Bo Li, & Xing Li, Propagation of non-Wentzel-Kramers-BrillouinAlfven waves in amulticomponentsolar wind with differential ion flow,ApJ, 661(2), 1222-1233 (2007)

Bo Li,ShadiaRifaiHabbal, and Xing Li, Angular momentum transport and proton–alpha particle differential streaming in the solar wind,ApJ, 661(1), 593-601 (2007)

X. Li, Q.-M. Lu, &B. Li, Ion pickup by finite amplitude parallel propagating Alfven waves,ApJLetters, 661(1), L105-L108 (2007)

B. Li, & X. Li, Effects of alpha particles on the angular momentum loss from the Sun, A&A, 456(1), 359-365 (2006)

N.Labrosse, X. Li, &B. Li, On the Lyman alpha and beta lines in solar coronal streamers, A&A, 455(2), 719-723 (2006)

B. Li, X. Li, & N.Labrosse, A global 2.5-dimensional three fluid solar wind model with alpha particles, Journal of Geophysical Research(JGR), 111, A08106 (2006)

S. T. Wu,B. Li, S. Wang, &HuinanZheng, A three-dimensional analysis of global propagation ofMagnetohydrodynamic(MHD) waves in a structured solar atmosphere, JGR, 110, A11102 (2005)

Bo Li, X. Li, Y.-Q.Hu, &ShadiaR.Habbal, A two-dimensional Alfven wave-driven solar wind model with proton temperature anisotropy, JGR, 109, A07103 (2004)

 

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