Tekijä: Gang Li (ed.); Qiang Hu (ed.); Olga Verkhoglyadova (ed.); Gary Zank (ed.); R.P. Lin (ed.); J. Luhmann (ed.) Kustantaja: American Institute of Physics (2008) Saatavuus: Loppuunmyyty.
Tekijä: Jacob Heerikhuisen (ed.); Gang Li (ed.); Nikolai Pogorelov (ed.); Gary P. Zank (ed.) Kustantaja: American Institute of Physics (2012) Saatavuus: Loppuunmyyty.
Tekijä: Qiang Hu (ed.); Gang Li (ed.); Gary P. Zank (ed.); Xianzhi Ao (ed.); James H Adams (ed.); Olga Verkhoglyadova (ed.) Kustantaja: American Institute of Physics (2012) Saatavuus: Loppuunmyyty.
Tekijä: Kyandoghere Kyamakya (ed.); Wolfgang A. Halang (ed.); Wolfgang Mathis (ed.); Jean Chamberlain Chedjou (ed.); Zhong Li (ed.) Kustantaja: Springer (2013) Saatavuus: Noin 17-20 arkipäivää
Tekijä: Wenjia Niu (ed.); Gang Li (ed.); Jiqiang Liu (ed.); Jianlong Tan (ed.); Li Guo (ed.); Zhen Han (ed.); Lynn Batten (ed.) Kustantaja: Springer (2015) Saatavuus: Noin 17-20 arkipäivää
Tekijä: Ding-Geng Chen (ed.); Zhezhen Jin (ed.); Gang Li (ed.); Yi Li (ed.); Aiyi Liu (ed.); Yichuan Zhao (ed.) Kustantaja: Springer (2018) Saatavuus: Noin 17-20 arkipäivää
Tekijä: Ding-Geng Chen (ed.); Zhezhen Jin (ed.); Gang Li (ed.); Yi Li (ed.); Aiyi Liu (ed.); Yichuan Zhao (ed.) Kustantaja: Springer (2019) Saatavuus: Noin 17-20 arkipäivää
Tekijä: V. S. Shankar Sriram (ed.); V. Subramaniyaswamy (ed.); N. Sasikaladevi (ed.); Leo Zhang (ed.); Lynn Batten (ed.); Gang Li Kustantaja: Springer (2019) Saatavuus: Noin 17-20 arkipäivää
Tekijä: Xiangfeng Luo (ed.); Marc Spaniol (ed.); Lizhe Wang (ed.); Qing Li (ed.); Wolfgang Nejdl (ed.); Wu Zhang (ed.) Kustantaja: Springer (2010) Saatavuus: Noin 17-20 arkipäivää
All papers have been peer-reviewed. Our star is a very effective particle accelerator. Energies up to GeVs have been observed in Solar energetic particle events. These events are often associated with solar flares and/or Coronal Mass Ejections. Understanding how particles are accelerated in these phenomena has been an outstanding problem in space plasma physics for a long time. Part of the reason is its practical (e.g. Space weather) and fundamental (cosmic ray origin) importance. In this conference we review recent progresses on this problem, with a balance between observations, theories and numerical simulations. Specific topics include 1) particle acceleration at flare site, 2) turbulence properties of the solar wind, 3) particle acceleration and transport in the inner heliosphere, 4) particle acceleration at the termination shock and heliosheath, and 5) particle acceleration at supernova remnant shocks.
