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Solar-terrestrial Magnetic Activity and Space Environment

Proceedings of the COSPAR Colloquium on Solar-Terrestrial Magnetic Activity and Space Environment (STMASE) Held in the NAOC in Beijing, China, September 10-12, 2001

By: H.N. Wang (Editor), R.L. Xu (Editor)

Hardcover

Published: 4th December 2002
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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 areas of the solar-terrestrial magnetic activity and space environment studies, including study on solar surface magnetism; solar magnetic activity, dynamical response of the heliosphere; space weather prediction; and space environment exploration and monitoring. A hot topic of space research, CMEs, which are widely believed to be the most important phenomenon of the space environment, is discussed in many papers. Other papers show results of observational and theoretical studies toward better understanding of the complicated image of the magnetic coupling between the Sun and the Earth, although little is still known little its physical background. Space weather prediction, which is very important for a modern society expanding into out-space, is another hot topic of space research. However, a long way is still to go to predict exactly when and where a disaster will happen in the space. In that sense, there is much to do for space environment exploration and monitoring. The manuscripts submitted to this Monograph are divided into the following parts: (1) solar surface magnetism, (2) solar magnetic activity, (3) dynamical response of the heliosphere, (4) space environment exploration and monitoring; and (5) space weather prediction. Papers presented in this meeting but not submitted to this Monograph are listed by title as unpublished papers at the end of this book.

Preface
Solar Surface Magnetism
Magnetic Reconnection in the Solar Lower Atmosphere
Small-Scale Magnetic Structure in the Photosphere
Sunspot Dynamics and Coronal Heating
Solar Coronal Activity and Evolution of the Magnetic Field
The Sun-as-Star Magnetic Field: Results of Stokesmeter Measurements in Different Spectral Lines
Useful Aspects of Chromospheric Magnetic Field Data
Configurations of Magnetic Fields in Solar Active Regions
Reversed Polarity Structures and Powerful X5.7/3b Flare on July 14, 2000,
Properties of Twist of Solar Bipolar Magnetic Fields
Helicity Evolution of a Spot
The Distribution of Magnetic Shear of Solar Active Regions From 1995 to 2000
The Evolution Rate of Small Solar Active Regions and Its Temporal and Spatial Variations
Correcting the Projection Effects of Solar Vector Magnetogram
The Application of Magnetic Line Ratio Method to Magnetographic Observations of Large-Scale Solar Magnetic Fields
The Primary Design of A 1-Meter Infrared Solar Telescope
Developing Huairou web Site
Solar Magnetic Activity
Lower Energy Cutoff of Nonthermal Electrons Derived From Batse/Cgro Hard X-Ray
Non-LTE Inversion of an Ha Flaring Loop
Magnetic Flux Cancellation Associated with Coronal Mass Ejections
Dip-Like Magnetic Field Structure Seen in Solar Prominences
Common Characteristics of CMEs and Blobs: a New View of Their Possible Origin
Statistical Studies of Filament Disappearances and CMEs
Catastrophic Behavior of Coronal Magnetic Flux Ropes in Partially Open Magnetic Fields
Coronal Response to the Emergence of New Magnetic Flux
Constraints on Models of the Initiation of Coronal Mass Ejections
What Can We Learn From Constructing CME Models
A Dual-Loop Initiation Model for Coronal Mass Ejections
Coronal Mass Ejections From the Corona to the Interplanetary Medium
Relation Between Coronal Mass Ejections and their Interplantary Counterparts
A Manifestation of Magnetic Fluxes in Microwave Emission of the Solar Corona
Statistical Properties of Radio-Rich Coronal Mass Ejections
The Broadening Cause of the CaXIX Resonace Line in Solar Flares
Dynamical Features of the Dipole Magnetic Fields Generated Two X-Ray Coronal Mass Ejections and Type IVmicro
S-Shaped Magnetic Field Generated an Extra Large Type IVmicro; Burst and Coronal Mass Ejection
Centimetric Type N and Type M Bursts
Role of Hydrogen and Deuterium in Energy Release From the Solar Flare: Comment on Neupert Effect
Analysis of the January 6-11, 1997, Coronal Mass Ejection
Dynamical Response of the Heliosphere
Analysis of Lasco Observations of Streamer Blowout Events
Table of Contents provided by Publisher. All Rights Reserved.

ISBN: 9780080441108
ISBN-10: 0080441106
Series: COSPAR
Audience: Professional
Format: Hardcover
Language: English
Number Of Pages: 474
Published: 4th December 2002
Publisher: Elsevier Science & Technology
Dimensions (cm): 18.0 x 26.5  x 2.7
Weight (kg): 1.116