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Waves & oscillations in the solar atmosphere : heating and magneto-seismology : proceedings of the 247th symposium of the International Astronomical Union held in Porlamar, Isla de Margarita Venezuela, September 17-22, 2007 / edited by Robert Erdélyi and César A. Mendoza-Briceño.

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Corporate Author:
International Astronomical Union. Symposium (247th : 2007 : Porlamar, Venezuela)
Language:
English.
Publication date:
2008
Imprint:
Cambridge ; New York : Cambridge University Press, 2008.
Format:
  • Book, Conference Proceedings
  • xviii, 378 p. : ill. ; 26 cm.
Title Variation:
Waves and oscillations in the solar atmosphere
Proceedings of the 247th symposium of the International Astronomical Union
Bibliography:
Includes bibliographical references and index.
Contents:
  • Preface-- Organizing committee-- Conference participants-- Address by the Scientific Organizing Committee R. Erdelyi-- Progress in coronal seismology B. Roberts-- Session 1. Waves and oscillations in solar and stellar interior Robert Erdelyi-- Session 2. Coupling of global solar and stellar motions into the lower atmosphere Bernard Roberts-- Session 3. Seismology of the lower solar atmosphere and stellar chromospheres Siraj S. Hasan-- Session 4. Seismology of open versus closed magnetic structures Marcel Goossens-- Session 5. Prominence seismology Jose Luis Ballester-- Session 6. Dynamical processes and coupling in the magnetic atmosphere of Sun and stars Miguel Ibanez-- Session 7. Wave-particle interactions in magnetized plasmas Cesar A. Mendoza-Briceno-- Session 8. Solar and stellar global coronal seismology Viggo Hansteen-- Session 9. Fundamental physical processes in coronae: waves, turbulence, reconnection Saku Tsuneta-- Session 10. Waves and instabilities in atmospheric plasmas Arnold O. Benz-- Summary of meeting Cesar A. Mendoza-Briceno-- Concluding remarks A. O. Benz-- Late papers-- Author index.
  • (source: Nielsen Book Data)
Publisher's Summary:
IAU Symposium 247 addresses the latest discoveries on magnetic waves and oscillations, observed recently in the atmosphere of the Sun. The energy sources which maintain the extraordinarily high temperature of the Sun's outer coronal layer continue to fascinate solar researchers. It is now clear that the ubiquitous magnetic fields in the solar atmosphere are the crucial ingredient to understanding the solar corona. These proceedings of IAU S247 contain a selection of presentations and reviews made by internationally renowned scientists on the solar heating enigma and magneto-seismology of the solar atmosphere. It emphasizes magnetic wave and oscillation observations in different observational bands, consolidation of the theory and the observational findings, and observations with new and future solar missions.
(source: Nielsen Book Data)
Contributor:
Erdélyi, R. (Robertus)
Mendoza-Briceño, César A.
Series:
IAU symposium proceedings series, 1743-9213 ; no. 247
IAU symposium and colloquium proceedings series no. 247.
Subjects:
ISBN:
9780521874694
0521874696

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