Positions: | Professor |
---|---|
Academic Title: | Professor |
E-mail: | bltan@nao.cas.cn |
Mailing Address: | Baolin Tan |
Education:
1983.9-1987.6, B.S. in Geology, China University of Geology in Wuhan
2000.9-2003.6, M.S. in Nuclear Fusion Plasma Physics, South-western Institute of Physics, Chengdu
2004.2-2006.6, PhD in Astrophysics, Graduate School of the Chinese Academy of Sciences (Purple Mountain Observatory of Chinese Academy of Sciences, Nanjing)
Career History:
1987.6-1995.8, Assistant Engineer, Metallurgical Geological Prospecting Bureau in Shandong
1995.8-2000.8, Engineer, Metallurgical Geological Prospecting Bureau in Shandong
2003.6-2004.2, Assistant Prof., Southwestern Institute of Physics, Chengdu
2006.6-2015.4, Associate Prof., National Astronomical Observatories of Chinese Academy of Sciences, Beijing
2015.4-present, Prof., National Astronomical Observatories of Chinese Academy of Sciences, Beijing.
Solar radio astronomy: physics of solar radio spectral fine structures, solar small-scale bursts and the related turbulence, precursors of solar flares, particle accelerations
Plasma astrophysicsSolar and stellar coronal heating mechanism, triggering mechanism of astro-plasma instabilities and energy release processes, physics of multi-timescale solar cycles
I demonstrated a series of solar microwave QPP, zebra patterns, revised type IIIs, and small-scale microwave bursts, and proposed theoretical models of tearing-mode oscillation in current-carrying flaring loops to explain these observations.
I also investigated the solar cycles with multi-timescale, including the 11-year, 51.5 year, and 103 year, and proposed that these periodicities dominated the forthcoming solar cycles.
I proposed a theoretical model of magnetic-gradient pumping (MGP) to explain the coronal heating and the formation of solar jets.
Tan B.L., Yu Z.Q., Huang J., Tan C.M., & Zhang Y., Very Long-period Pulsations before the Onset of Solar Flares, 2016, ApJ, 833, 206
Tan B.L., Karlicky M., Meszarosova H. & Huang G.L., Diagnose physical conditions near the flare energy-release sites from observations of solar microwave Type III bursts, 2016, RAA, 16,74
Tan B.L., Coronal Heating Driven by Magnetic-gradient Pumping Mechanism in Solar Plasmas, 2014, ApJ, 795, 140
Tan B.L., Small Scale Microwave Bursts in Long-duration Solar Flares, 2013, ApJ, 773, 165
Tan B.L. & Tan C.M., Microwave quasi-periodic pulsation with millisecond bursts in a solar flare on 2011 August 9, 2012, ApJ, 749, 28
Tan B.L., Multi-timescale Solar Cycles and their Possible Implications, 2011, Ap&SS, 332, 65
Tan B.L., A Physical Explanation on Solar Microwave Zebra Pattern with the Current-carrying Plasma Loop Model, 2010, Ap&SS, 325, 251
Tan B.L., Observable Parameters and Their Possible Implications of the Solar Microwave Pulsating Structures, 2008, Sol. Phys., 253,117