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Solar-Terrestrial Magnetic Activity and Space Environment Book

Solar-Terrestrial Magnetic Activity and Space Environment
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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
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  • Solar-Terrestrial Magnetic Activity and Space Environment
  • Written by author Huaning Wang, R. L. Xu, COSPAR Staff
  • Published by A Pergamon Title, 2002/11/20
  • 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
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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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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

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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

Solar-Terrestrial Magnetic Activity and Space Environment

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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

Solar-Terrestrial Magnetic Activity and Space Environment

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