Editorial: solar radiophysics—recent results on observations and theories  

作　　者：Valery M.Nakariakov Larisa K.Kashapova Yi-Hua Yan 

机构地区：[1]Centre for Fusion,Space and Astrophysics,Department of Physics,University of Warwick,CV47AL,UK [2]School of Space Research,Kyung Hee University,Yongin,446-701,Gyeonggi,Korea [3]Central Astronomical Observatory at Pulkovo of RAS,St Petersburg 196140,Russia [4]Institute of Solar-Terrestrial Physics,Russian Academy of Sciences,Siberian Branch,126a Lermontov st.,664033,Irkutsk,Russia [5]Key Laboratory of Solar Activity,National Astronomical Observatories,Chinese Academy of Sciences

出　　处：《Research in Astronomy and Astrophysics》2014年第7期I0001-I0006,共6页天文和天体物理学研究（英文版）

基　　金：supported by the Marie Curie PIRSES-GA-2011295272"Radiophysics of the Sun"project;support by the National Natural Science Foundation of China(Grant No.11221063);MOST Grant 2011CB811401;the National Major ScientificEquipment R&D Project ZDYZ2009-3

摘　　要：Solar radiophysics is a rapidly developing branch of solar physics and plasma astrophysics. Solar radiophysics has the goal of analyzing observations of radio emissions from the Sun and understanding basic physical processes operating in quiet and active regions of the solar corona. In the near future, the commissioning of a new generation of solar radio observational facilities, which include the Chinese Spectral Radio Heliograph（CSRH） and the upgrade of the Siberian Solar Radio Telescope（SSRT）, and the beginning of solar observations with the Atacama Large Millimeter/submillimeter Array（ALMA）, is expected to bring us new breakthrough results of a transformative nature. The Marie-Curie International Research Staff Exchange（MC IRSES） “RadioSun” international network aims to create a solid foundation for the successful exploitation of upcoming solar radio observational facilities, as well as intensive use of the existing observational tools, advanced theoretical modeling of relevant physical processes and observables, and training a new generation of solar radio physicists. The RadioSun network links research teams from China,Czech Republic, Poland, Russia and the UK. This mini-volume presents research papers based on invited reviews and contributed talks at the 1st RadioSun workshop in China. These papers cover a broad range of research topics and include recent observational and theoretical advances in solar radiophysics, MHD seismology of the solar corona, physics of solar flares, generation of radio emission, numerical modeling of MHD and plasma physics processes, charged-particle acceleration and novel instrumentation.Solar radiophysics is a rapidly developing branch of solar physics and plasma astrophysics. Solar radiophysics has the goal of analyzing observations of radio emissions from the Sun and understanding basic physical processes operating in quiet and active regions of the solar corona. In the near future, the commissioning of a new generation of solar radio observational facilities, which include the Chinese Spectral Radio Heliograph（CSRH） and the upgrade of the Siberian Solar Radio Telescope（SSRT）, and the beginning of solar observations with the Atacama Large Millimeter/submillimeter Array（ALMA）, is expected to bring us new breakthrough results of a transformative nature. The Marie-Curie International Research Staff Exchange（MC IRSES） “RadioSun” international network aims to create a solid foundation for the successful exploitation of upcoming solar radio observational facilities, as well as intensive use of the existing observational tools, advanced theoretical modeling of relevant physical processes and observables, and training a new generation of solar radio physicists. The RadioSun network links research teams from China,Czech Republic, Poland, Russia and the UK. This mini-volume presents research papers based on invited reviews and contributed talks at the 1st RadioSun workshop in China. These papers cover a broad range of research topics and include recent observational and theoretical advances in solar radiophysics, MHD seismology of the solar corona, physics of solar flares, generation of radio emission, numerical modeling of MHD and plasma physics processes, charged-particle acceleration and novel instrumentation.

关 键 词：EDITORIALS notices -- Sun： corona -- Sun： radio radiation -- Sun： flares 

分 类 号：P182.24[天文地球—天文学]