Solar-Terrestrial Magnetic Activity and Space EnvironmentElsevier, 2002. gada 20. nov. - 474 lappuses 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 Papers presented in this meeting but not submitted to this Monograph are listed by title as unpublished papers at the end of this book. |
Saturs
83 | |
Dynamical Response of the Heliosphere | 199 |
Space Exploration and Environment | 331 |
Space Weather Prediction | 373 |
Author Index | 453 |
List of Participants | 457 |
List of Unpublished Papers | 459 |
Citi izdevumi - Skatīt visu
Solar-terrestrial Magnetic Activity and Space Environment: Proceedings of ... H. Wang,Ronglan L. Xu Ierobežota priekšskatīšana - 2002 |
Bieži izmantoti vārdi un frāzes
acceleration active regions associated Astron Astrophys auroral Bastille Day Beijing bursts Chen China chromospheric coronagraph coronal mass ejections correlation current sheet cusp density distribution Dst index dynamic effect electron emission energetic particles energy equation eruption evolution field lines Figure filament flux cancellation flux rope forecast frequency frontside full halo full halo CMEs geoeffective geomagnetic storms Geophys Gopalswamy hard X-ray helicity heliosphere high latitude images indices interplanetary ionosphere LASCO loop magnetic clouds magnetic field magnetic flux magnetic interface magnetic reconnection magnetograms magnetopause magnetosphere maximum measurements Observatory observed orbit panel parameters phase photosphere plasma polarity power law prediction proton radiation radio ring current shear shock shows SKAWs solar activity solar cycle solar flare Solar Phys solar wind space weather spacecraft spectral speed sprites streamer structure substorms sunspot sunspot numbers variations vector magnetograms velocity Wang Zhang
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128. lappuse - The National Center for Atmospheric Research is sponsored by the National Science* Foundation.
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