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Preface | ||
Magnetic Reconnection in the Solar Lower Atmosphere | 3 | |
Small-Scale Magnetic Structure in the Photosphere: Relevance to Space Weather Phenomena | 9 | |
Sunspot Dynamics and Coronal Heating | 19 | |
Solar Coronal Activity and Evolution of the Magnetic Field | 27 | |
The Sun-as-a- Star Magnetic Field: Results of Stokesmeter Measurements in Different Spectral Lines | 33 | |
Useful Aspects of Chromospheric Magnetic Field Data | 37 | |
Configurations of Magnetic Fields in Solar Active Regions | 41 | |
Reversed Polarity Structures and Powerful X5.7/3B Flare on July 14, 2000 | 45 | |
Properties of Twist of Solar Bipolar Magnetic Fields | 51 | |
Helicity Evolution of a Spot | 55 | |
The Distribution of Magnetic Shear of Active Regions From 1995 to 2000 | 59 | |
The Evolution Rate of Small Solar Active Regions and Its Temporal and Spatial Variations | 63 | |
Correcting the Projection Effects of Solar Vector Magnetogram | 67 | |
Applications of Magnetic Line Ratio Method to Magnetographic Observations of Large-Scale Solar Magnetic Fields | 71 | |
The Primary Design of A 1-Meter Infrared Solar Telescope | 75 | |
Huairou Data On Line | 79 | |
Lower Energy Cutoff of Nonthermal Electrons Derived From Batse/CGRO Hard X-Ray | 85 | |
Non-LTE Inversion of an H[alpha] Flaring Loop | 89 | |
Magnetic Flux Cancellation Associated with Coronal Mass Ejections | 93 | |
Dip-Like Magnetic Field Structure Seen in Solar Prominences | 103 | |
Common Characteristics of CMEs and Blobs: a New View of Their Possible Origin | 109 | |
Statistical Studies of Filament Disappearances and CMEs | 113 | |
Catastrophic Behavior of Coronal Magnetic Flux Ropes in Partially Open Magnetic Fields | 117 | |
Coronal Response to the Emergence of New Magnetic Flux | 125 | |
Initiation of Coronal Mass Ejections | 129 | |
What Can We Learn From Constructing CME Models | 137 | |
A Dual-Loop Initiation Model for Coronal Mass Ejections | 145 | |
Coronal Mass Ejections From the Corona to the Interplanetary Medium | 149 | |
Relation Between Coronal Mass Ejections and their Interplanetary Counterparts | 157 | |
A Manifestation of Magnetic Fluxes in Microwave Emission of the Solar Corona | 165 | |
Statistical Properties of Radio-Rich Coronal Mass Ejections | 169 | |
The Broadening Cause of the CaXIX Resonace Line in Solar Flares | 173 | |
Dynamical Features of the Dipole Magnetic Fields Generated Two X-Ray Coronal Mass Ejections and Type IV[mu] Burst | 175 | |
S-Shaped Magnetic Field Generated an Extra Large Type IV[mu] Burst and Coronal Mass Ejection | 179 | |
Solar Centimetric Type N and Type M Bursts | 183 | |
Role of Hydrogen and Deuterium in Energy Release From the Solar Flare: Comment on Neupert Effect | 189 | |
Analysis of the January 6-11, 1997, CME Event | 193 | |
Analysis of Lasco Observations of Streamer Blowout Events | 201 | |
The Geoeffectiveness of Frontside Full Halo Coronal Mass Ejections | 209 | |
The Heliospheric Magnetic Field Probed with Fast Charged Particles | 217 | |
Evolution of the Bastille Day High-Speed Stream | 225 | |
Ensemble and Time Averages: the Missing Diamagnetic Effect | 233 | |
The Global Significance of the CEP Events | 239 | |
Effects of Electron Pressure Gradient in Magnetic Reconnection | 251 | |
The Effect of Geomagnetic Disturbances on Ecosystem | 255 | |
Relationship Between the Cumulative AL and Dst Indices During Magnetic Storms and the UT Variations of the Dst Index | 259 | |
Solar Wind Density and the Auroral Electrojets During Geomagnetic Storms | 263 | |
A Cone Model for Coronal Mass Ejections | 267 | |
Injection of Intense Storm Ring Current Ions | 271 | |
Heliospheric Magnetic Fields and Particle Transport | 275 | |
Geomagnetic Disturbances as Probabilistic Nonlinear Processes | 281 | |
Fine Structure of Sprites and Proposed Global Observations | 287 | |
Night-Time Behavior of 630 Nm Emission in Mid-Latitude Auroras during Strong Magnetic Storms | 295 | |
Doppler Effects in the High-Latitude Ionospere during Observations Geomagnetic Pulsations | 299 | |
Time-Variation of Periodic Components of Yearly Sunspot Numbers | 307 | |
A New Model for Evaluation of the Electromagnetic Energy Flux into an Open Night side Magnetosphere | 311 | |
Numerical Modeling the High-Latitude Ionosphere | 315 | |
Basic Cause of Solar Magnetic Activity Solar Motion or Gyromagnetic Effect | 327 | |
Some Implications of the Interball Studies for Space Weather | 333 | |
Solar Radio Bursts and Fine Structures in the Range of 1.0-7.6 GHz on 14 July 2000 | 345 | |
On the Solar Radio Spectro-Interferometry at Low Frequency | 349 | |
Drift Shell Tracing and Secular Variation of inner Radiation Environment in the Saa Region | 353 | |
Energetic Ions in the High Latitude Magnetosphere During the Leading Phase of Acme | 359 | |
Space Environment Data Acquisition Equipment - Attached Payload on the International Space Station | 365 | |
Space Environment Data Acquisition Equipment on Board Mission Demonstration Test Satellite-1 | 369 | |
Space Weather: The Scientific Forecast | 375 | |
Space Weather Effects and how Soho has Improved the Warnings | 385 | |
Implementation and Verification of the Chen Prediction Technique for Forecasting Large Nonrecurring Storms | 393 | |
An Applicable Method for Long-Term Solar Cycle Predictions | 397 | |
Real-Time Space Weather Forecasting Driven by Solar Observations | 401 | |
A New Mechanism for Auroral Electron Acceleration by Nonlinear KAW | 409 | |
Geomagnetic Activity and Solar-Cycle Dependence of the Ring Current Ions | 421 | |
The Application of Non-Linear Filtering Methods to the Forecast of Geomagnetic Indices | 427 | |
Prediction of Relativistic Electron Fluence Using Magnetic Observatory Data | 439 | |
Space Weather Aspects of the ESA Solar Orbiter Mission | 443 | |
Effects of Hysteresis in Solar Cycle Variations Between Flare Index and some Solar Activity Indicators | 447 | |
Author Index | 453 | |
List of Participants | 457 | |
List of Unpublished Papers | 459 |
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Add Solar-Terrestrial Magnetic Activity and Space Environment, The COSPAR Colloquium on Solar-Terrestrial Magnetic Activity and Space Environment (STMASE) was held in the National Astronomy Observatories of Chinese Academy of Sciences (NAOC) in Beijing, China in September 10-12, 2001. The meeting was focused on five , Solar-Terrestrial Magnetic Activity and Space Environment to the inventory that you are selling on WonderClubX
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Add Solar-Terrestrial Magnetic Activity and Space Environment, The COSPAR Colloquium on Solar-Terrestrial Magnetic Activity and Space Environment (STMASE) was held in the National Astronomy Observatories of Chinese Academy of Sciences (NAOC) in Beijing, China in September 10-12, 2001. The meeting was focused on five , Solar-Terrestrial Magnetic Activity and Space Environment to your collection on WonderClub |