欢迎您！东篱公司
退出
-
申报数据库
-
立项数据库
-
成果数据库
-
项目获奖数据库
中文摘要：
太阳是距离地球最近的恒星,不仅对于日地空间环境具有重要的影响,而且作为独一无二的天然等离子体实验室,有助于理解宇宙中电磁相互作用的基本过程.螺度作为描述矢量场属性的基本参量,在理解太阳物理研究的核心课题——太阳磁场的起源和磁场能量的释放机制方面具有重要意义.本文探讨了螺度的基本概念（包括磁螺度、电流螺度、运动学螺度等）,以及我国太阳物理学家在螺度研究中的主要进展,并对未来太阳物理中螺度研究的问题做了一些探讨.
英文摘要：
The Sun is the nearest star to the Earth. The Sun not only affects the environment of interplanetary space but, as a unique large-scale natural plasma laboratory, also helps us understand the basic process of electromagnetic interaction in the universe. Helicity is a basic parameter to describe the properties of vector fields. It is important in understanding the origin of the solar magnetic field and the release mechanism of solar magnetic energy, which are key subjects in solar physics. In this paper, we discuss the basic concepts of helicity （including magnetic helicity, current helicity, and kinematic helicity） and major advances in helicity research. Based on these information, we raise new open questions regarding the helicity research of solar physics.
同期刊论文项目
同项目期刊论文
LARGE-SCALE MAGNETIC HELICITY FLUXES ESTIMATED FROM MDI MAGNETIC SYNOPTIC CHARTS OVER THE SOLAR CYCL
Effects of thenon-radial magnetic field on measuring magnetic helicity transport across thesolar pho
Correlation between CME occurrence rate and current helicity in global magnetic field of solar cycle
Analysis on Correlations between Subsurface Kinetic Helicity and Photospheric Current Helicity in Ac
Relationship between powerful flares and dynamic evolution of the magnetic field at the solar surfac
Magnetic-Field Variations in the Active Region NOAA 10486 and Their Relationship to X-Ray Flares and
Tracking Back the Solar Wind to Its Photospheric Footpoints from Wind Observations - A Statistical S
Effects of the Scatter in Sunspot Group Tilt Angles on the Large-scale Magnetic Field at the Solar S
Effects of Alfvén Waves on Electron Cyclotron Maser Emission in Coronal Loops and Solar Type I Radio
Observations of a Quasi-Periodic Fast Propagating Magnetosonic Wave in Multi-Wavelength and Its Inte
Coronal Heating By the Interaction between Emerging Active Regions and the Quiet Sun Observed By the
Improved magnetogram calibration of Solar Magnetic Field Telescope and its comparison with the Helio
The dependence of flares on the magnetic classification of the source regions in solar cycles 22-23,
Periodicity of the solar radius revisited by using empirical mode decomposition and the Lomb–Scargle
Dark Ribbons Propagating and Sweeping across Extreme Ultraviolet Structures after Filament Eruptions
The Relationship between the Particle Injection Rate and the Dispersion of the Scattering Angular Di
Magnetic Reconnection: From “Open” Extreme-ultraviolet Loops to Closed Post-flare Ones Observed by S
Dynamics of Flare Processes and Variety of the Fine Structure of Solar Radio Emission over a Wide Fr
Some tests and improvements to the VFISV: Very Fast Inversion of the Stokes Vector for the Helioseis
Multi-channel observations of plasma outflows and the associated small-scale magnetic field cancella
Well-observed Dynamics of Flaring and Peripheral Coronal Magnetic Loops during an M-class Limb Flare
Relationship between extreme ultraviolet microflares and small-scale magnetic fields in the quiet Su
Quasi-periodic Slipping Magnetic Reconnection During an X-class Solar Flare Observed by the Solar Dy
Evolution of Relative Magnetic Helicity: Method of Computation and Its Application to a Simulated So
Three-Dimensional Nonlinear Force-Free Field Reconstruction of Solar Active Region 11158 by Direct B
Forced Field Extrapolation: Testing a Magnetohydrodynamic (MHD) Relaxation Method with a Flux-rope E
Effects of the Non-Radial Magnetic Field on Measuring Magnetic Helicity Transport across the Solar P
The contracting and unshearing motion of flare loops in the X7.1 flare on 2005, January 20 during it
期刊信息
位置：