位置：成果数据库 > 期刊 > 期刊详情页
Quasar Formation and Energy Mechanism in Black Hole Universe
  • 期刊名称：Progress in Phys.
  • 时间：0
  • 页码：48-
  • 相关项目：空间天气的太阳驱动源研究
作者： Zhang, T. X.|
同期刊论文项目
空间天气的太阳驱动源研究
期刊论文 79 会议论文 4
同项目期刊论文
An investigation of magnetic field distortions in accretion discs around neutron stars: II. Analysis
Global analysis of active longitudes of sunspots
The Solar Cycle: a new prediction technique based on logarithmic values
Recent progress of research and operational activities of solar weather forecasting at NAOC
THREE-DIMENSIONAL SHAPE AND EVOLUTION OF TWO ERUPTIVE FILAMENTS
GRAVITATIONAL FIELD SHIELDING AND SUPERNOVA EXPLOSIONS
A statistical study on the brightening propagation of post-flare loops
Correlations Between CME Parameters and Sunspot Activity
Emerging dimmings of active regions observed by SDO
The Shape of Solar Cycle Described by a Modified Gaussian Function
The relationships of solar flares with both sunspot and geomagnetic activity
The Turning Point for the Recent Acceleration of the Universe with a Cosmological Constant
Recent Progress of Solar Weather Forecasting at NAOC, 2011, Advances in Geosciences
Gravitationless black holes
The correlation between solar and geomagnetic activity - Part 2: Long-term trends
Global analysis of active longitudes of solar X-ray flares
The correlation between solar and geomagnetic activity - Part 1: Two-term decomposition of geomagnet
Propagation of Moreton Waves
The Rotation Rates of Solar Magnetic Fields During Solar Cycles 21-aEuro parts per thousand 23
Fundamental Elements and Interactions of Nature: A Classical Unification Theory
Cosmic microwave background radiation of black hole universe
Does a low solar cycle minimum hint at a weak upcoming cycle?
Is a higher correlation necessary for a more accurate prediction?
The Relationship between Prediction Accuracy and Correlation Coefficient
The prediction method of similar cycles
A logistic model for magnetic energy storage in solar active regions
Correlation Function Analysis between Sunspot Cycle Amplitudes and Rise Times
Magnetohydrodynamic simulation of non-flux rope coronal mass ejections
THE PREDICTIVE POWER OF OHL';S PRECURSOR METHOD
Neutron Star Mass-Radius Relation with Gravitational Field Shielding by Scalar Field
The correlation between solar and geomagnetic activity - Part 3: An integral response model
UBIQUITOUS ROTATING NETWORK MAGNETIC FIELDS AND EXTREME-ULTRAVIOLET CYCLONES IN THE QUIET SUN
Solar Intranetwork Magnetic Elements: Intrinsically Weak or Strong?
Gravitational Field Shielding by Scalar Field and Type II Superconductors
A method of magnetosonic characteristics to correct the "rarefaction shocks" problem arising in ZEUS
Self-cancellation of Ephemeral Regions in the Quiet Sun.
Kinematics and amplitude evolution of global coronal extreme ultraviolet waves
Predicting the solar maximum with the rising rate
The kinematics of an untwisting solar jet in a polar coronal hole observed by SDO/AIA
Quantifying solar superactive regions with vector magnetic field observations