Editorial： solar radiophysics—recent results on observations and theories

• Published in: Research in astronomy and astrophysics 2014-07, Vol.14 (7), p.I0001-I0006
• Main Authors: Nakariakov, Valery M., Kashapova, Larisa K., Yan, Yi-Hua
• Format: Article
• Language: English
• Subjects: 天体物理学; 太阳射电望远镜; 太阳能; 无线电频谱; 物理过程; 研究成果; 磁流体力学; 编辑
• ISSN: 1674-4527; 2397-6209
• DOI: 10.1088/1674-4527/14/7/001

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.