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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 /

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 activ...

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Detalles Bibliográficos
Clasificación:Libro Electrónico
Autor Corporativo: COSPAR Colloquium on Solar-Terrestrial Magnetic Activity and Space Environment Beijing, China
Otros Autores: Wang, Huaning, Xu, R. L. (Ronglan L.)
Formato: Electrónico Congresos, conferencias eBook
Idioma:Inglés
Publicado: Amsterdam ; Boston : Pergamon, 2002.
Edición:1st ed.
Colección:COSPAR colloquia series ; v. 14.
Temas:
Acceso en línea:Texto completo
Texto completo
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MARC

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245 1 0 |a Solar-terrestrial magnetic activity and space environment :  |b 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 /  |c edited by Huaning Wang and Ronglan Xu. 
250 |a 1st ed. 
260 |a Amsterdam ;  |a Boston :  |b Pergamon,  |c 2002. 
300 |a 1 online resource (xii, 462 pages) :  |b illustrations 
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490 1 |a COSPAR colloquia series ;  |v v. 14 
505 0 0 |t Preface / Guoxiang Ai --  |g Section I.  |t Solar surface magnetism --  |t Magnetic reconnection in the solar lower atmosphere /  |r C. Fang, P.F. Chen, M.D. Ding --  |t Small-scale magnetic structure in the photosphere: Relevance to space weather phenomena /  |r V. Mart�inez Pillet --  |t Sunspot dynamics and coronal heating /  |r N. Hurlburt, D. Alexander --  |t Solar coronal activity and evolution of the magnetic field /  |r E.E. Benevolenskaya, A.G. Kosovichev, P.H. Scherrer --  |t The sun-as-a-star magnetic field: Results of stokesmeter measurements in different spectral lines /  |r M.L. Demidov, V.V. Zhigalov, V.S. Peshcherov, V.M. Grigoryev --  |t Useful aspects of chromospheric magnetic field data /  |r T. Sakurai, Debi Prasad Choudhary, P. Venkatakrishnan --  |t Configuration of magnetic field inferred from magnetogramsspace /  |r Hongqi Zhang --  |t Reversed polarity structures and powerful X5.7/3B flare on July 14,2000 /  |r Wei Li, Yuanyong Deng, Yihua Yan, Xinming Bao --  |t Properties of twist of solar bipolar magnetic fields /  |r Lirong Tian, Hongqi Zhang --  |t Helicity evolution of a spot /  |r Y. Liu, H. Zhang --  |t The distribution of magnetic shear of active regions from 1995 to 2000 /  |r J. Dun, H. Zhang, B. Zhang, R. Li --  |t The evolution rate of small solar active regions and its temporal and spatial variations /  |r A.A. Golovko --  |t Correcting the projection effects of solar vector magnetogram /  |r Hui Li --  |t Applications of magnetic line ratio method to magnetographic observations of large-scale solar magnetic fields /  |r R.M. Veretsky, M.L. Demidov --  |t The primary design of a 1-meter infrared solar telescope /  |r W.D. Cao, Z. Liu, B.X. Ye --  |t Huairou data on line /  |r Ganghua Lin. 
505 0 0 |6 880-01  |g Section III.  |t Dynamical response of the heliosphere --  |t Analysis of LASCO observations of streamer blowout events /  |r A. Vourlidas, R.A. Howard, J.S. Morrill, S. Munz --  |t The geoeffectiveness of frontside full halo coronal mass ejections /  |r X.P. Zhao --  |t The heliospheric magnetic field probed with fast charged particles /  |r Joe Giacalone --  |t Evolution of the bastille day high-speed stream /  |r Y.C. Whang, L.F. Burlaga --  |t Ensemble and time averages: The missing diamagnetic effect /  |r R. Steinitz --  |t The global significance of cep events /  |r Jiasheng Chen, Theodore A. Fritz --  |t Effects of electron pressure gradient in magnetic reconnection /  |r J.B. Cao, Z.W. Ma, G.C. Zhou, Z.X. Liu --  |t The effect of geomagnetic disturbances on ecosystem /  |r C.Y. Fan, Y.C. Lin --  |t Relationship between the cumulative AL and Dst indices during magnetic storms and the UT variations of the Dst index /  |r B.-H. Ahn, Ga-Hee Moon, Wei Sun, Y.D. Park, G.X. Chen --  |t Solar wind density and auroral electrojets during geomagnetic storms /  |r Y. Kamide, J.-H. Shue, M. Brittnacher --  |t A cone model for coronal mass ejections /  |r W. Liu, S.P. Plunkett, X.P. Zhao --  |t Injection of intense storm ring current ions /  |r L. Xie, Z.Y. Pu, B. Yu, S.Y. Fu, Q.G. Zong, J.N. Tu --  |t Heliospheric magnetic fields and particle transport /  |r Yu-Qing Lou --  |t Geomagnetic disturbances as probabilistic nonlinear processes /  |r Y. Watanabe, H. Shirai, Y. Kamide --  |t Fine structure of sprites and proposed global observations /  |r S.B. Mende, H.U. Frey, R.L. Rairden, Han-Tzong Su, R-R Hsu, T.H. Allin, T. Neubert, E.A. Gerken, U.S. Inan --  |t Night-time behavior of 630 nm emission in mid-latitude auroras during strong magnetic storms /  |r A.V. Mikhalev --  |t Doppler effects in the high-latitude ionospere during observations geomagnetic pulsations /  |r Yu. V. Lipko, A. Yu. Pashinin, R.A. Rakhmatulin --  |t Time-variation of periodic components of yearly sunspot numbers /  |r Yanben Han, Yonggang Han --  |t A new model for evaluation of the electromagnetic energy flux into an open nightside magnetosphere /  |r V.V. Shelomentsev --  |t Numerical modeling the high-latitude ionosphere /  |r A.V. Tashchilin, E.B. Romanova --  |t Basic cause of solar magnetic activity solar motion or gyromagnetic effect /  |r S.L. Dong. 
505 0 0 |g Section VI.  |t Space exploration and environment --  |t Some implications of the interball studies for space weather /  |r L. Zelenyi, G. Zastenker, A. Petrukovich, L. Chesalin, P. Dalin, M. Riazantseva, E. Ryazanova, E. Lakutina --  |t Solar radio bursts and fine structures in the range of 1.0-7.6 GHz on 14 July 2000 /  |r S.J. Wang, Y.H. Yan, Q.J. Fu --  |t On the solar radio spectro-interferometry at low frequency /  |r Yihua Yan, Qijun Guangli Huang, Zhihai Qin, Jian Zhan --  |t Drift shell tracing and secular variation of inner radiation environment in the SAA region /  |r Z.Y. Pu, L. Xie, X.H. Fang, W.X. Jiao, S.Y. Fu, Q.G. Zong --  |t Energetic ions in the high latitude magnetosphere during the leading phase of a CME /  |r Q.-G. Zong, T.A. Fritz, S.-Y. Fu, Z.-Y. Pu, P. Daly --  |t Space environment data acquisition equipment-attached payload on the international space station /  |r K. Koga, T. Goka, H. Matsumoto, H. Koshishi, Y. Kimoto, T. Kanamori, C. Kamakura, M. Ito, E. Endo --  |t Space environment data acquisition equipment on board mission demonstration test satellite-1 /  |r H. Koshiishi, H. Matsumoto, Y. Kimoto, H. Liu, T. Goka. 
505 0 0 |g Section V.  |t Space weather prediction --  |t Space weather: The scientific forecast /  |r H. Wang, P.T. Gallagher, V. Yurchyshyn --  |t Space weather effects and how soho has improved the warnings /  |r P. Brekke --  |t Implementation and verification of the chen prediction technique for forecasting large nonrecurrent storms /  |r C. Arge, S. Wahl, J. Chen, S. Slinker, V. Pizzo --  |t An applicable method for long-term solar cycle predictions /  |r J.L. Wang, Yanben Han, Jian-Cun Gong, Si-Qing Liu, Guiming Le, Jing-lan Sun --  |t Real-time space weather forecasting driven by solar observations /  |r C.D. Fry, W. Sun, C. Deehr, M. Dryer, Z. Smith, S.-I. Akasofu --  |t A new mechanism for auroral electron acceleration by nonlinear kaw /  |r Wu DeJin, Chao JihKwin, Lee LuoChuan, Feng XueShang --  |t Geomagnetic and solar cycle dependence of the ring current ions /  |r S.Y. Fu, Q.G. Zong, Z.Y. Pu, L. Xie --  |t The application of non-linear filtering methods to the forecast of geomagnetic indices /  |r R.F. Harrison, P.M. Drezet --  |t Prediction of relativistic electron fluence using magnetic observatory data /  |r H.-L. Lam --  |t Space weather aspects of the esa solar orbiter mission /  |r R.G. Marsden, B. Fleck --  |t Effects of hysteresis in solar cycle variations between flare index and some solar activity indicators /  |r A. �Ozg�u�c, T. Ata�c --  |t Author index --  |t List of participants --  |t List of unpublished papers. 
520 |a 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. 
504 |a Includes bibliographical references and index. 
588 0 |a Print version record. 
650 0 |a Solar magnetic fields  |v Congresses. 
650 0 |a Geomagnetism  |v Congresses. 
650 0 |a Space environment  |v Congresses. 
650 6 |a G�eomagn�etisme  |0 (CaQQLa)201-0012441  |v Congr�es.  |0 (CaQQLa)201-0378219 
650 6 |a Environnement spatial  |0 (CaQQLa)201-0016584  |v Congr�es.  |0 (CaQQLa)201-0378219 
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650 7 |a Space environment  |2 fast  |0 (OCoLC)fst01127673 
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700 1 |a Wang, Huaning. 
700 1 |a Xu, R. L.  |q (Ronglan L.) 
776 0 8 |i Print version:  |a COSPAR Colloquium on Solar-Terrestrial Magnetic Activity and Space Environment (2001 : Beijing, China).  |t Solar-terrestrial magnetic activity and space environment.  |b 1st ed.  |d Amsterdam ; Boston : Pergamon, 2002  |z 0080441106  |z 9780080441108  |w (DLC) 2002038158  |w (OCoLC)50859114 
830 0 |a COSPAR colloquia series ;  |v v. 14. 
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856 4 0 |u https://sciencedirect.uam.elogim.com/science/publication?issn=09642749&volume=14  |z Texto completo 
856 4 0 |u https://sciencedirect.uam.elogim.com/science/bookseries/09642749/14  |z Texto completo 
880 0 0 |6 505-01/(S  |g Section II.  |t Solar magnetic activity --  |t Lower energy cutoff of nonthermal electrons derived from BATSE/CGRO hard x-ray observations /  |r W.Q. Gan, Y.P. Li, J. Chang --  |t Non-LTE inversion of an Hα flaring loop /  |r M.D. Ding, Y. Liu, P.F. Chen, C. Fang --  |t Magnetic flux cancellation associated with coronal mass ejections /  |r Jingxiu Wang, Jun Zhang, Yuanyong Deng --  |t Dip-like magnetic structure seen in solar prominences /  |r H.S. Yun, S. Lee, J. Chae, J. Lee, G.S. Choe, J.H. Kim, Y.D. Park, P.R. Goode, H. Wang --  |t Common characteristic of CMEs and blobs: A new view of their possible origin /  |r V.G. Eselevich, M.V. Eselevich --  |t Statistical studies of filament disappearances and CMEs /  |r G. Yang, H. Wang --  |t Catastrophic behavior of coronal magnetic flux ropes in partially open magnetic fields /  |r Y.Q. Hu --  |t Coronal response to the emergence of new magnetic flux /  |r M. Zhang --  |t Initiation of coronal mass ejections: Constraints on models from observations /  |r Nariaki V. Nitta --  |t What can we learn from constructing CME models: Magneric interface /  |r Jun Lin, Jingxiu Wang --  |t A dual-loop initiation model for coronal mass ejections /  |r A.M. Uralov, S.V. Lesovoi, V.G. Zandanov --  |t Coronal mass ejections to the interplanetary medium /  |r M. Pick --  |t Relation between coronal mass ejections and their interplanetary counterparts /  |r N. Gopalswamy --  |t A manifestation of magnetic fluxes in microwave emission of the solar corona /  |r B.V. Agalakov, B.I. Lubyshev, D.V. Prosovetsky, G.V. Rudenko, G. Ya. Smolkov, A.M. Uralov --  |t Statistical properties of radio-rich coronal mass ejections /  |r N. Gopalswamy, S. Yashiro, G. Michalek, M.L. Kaiser, R.A. Howard, J.-L. Bougeret --  |t The broadening cause of the CaXIX resonace line in solar flares /  |r Y.P. Li, W.Q. Gan --  |t Dynamical features of the dipole magnetic fields generated two X-ray coronal mass ejections and type IVμ burst /  |r S.C. Ji --  |t S-shaped magnetic field generated an extra large type IVμ burst and coronal mass ejection /  |r S.C. Ji --  |t Solar centimetric type N and type M bursts /  |r Min Wang, Qijun Fu, Ruixiang Xie --  |t Role of hydrogen and deuterium in energy release from the solar flare: Comment on Neupert effect /  |r Run-bao Lu --  |t Analysis of the January 6-11, 1997, CME event /  |r Y.Q. Wu, Y.H. Tang, Y. Dai, G.P. Wu.