THE DYNAMIC SUN ASTROPHYSICS AND SPACE SCIENCE LIBRARY VOLUME 259 EDITORIAL BOARD Chairman W. B. BURTON, Sterrewacht, Leiden, P.O. Box 9513, 2300 RA Leiden, The Netherlands [email protected] Executive Committee J. M. E. KUIJPERS, Faculty of Science, Nijmegen, The Netherlands E. P. J. VAN DEN HEUVEL, Astronomical Institute, University of Amsterdam, The Netherlands H. VAN DER LAAN, Astronomical Institute, University of Utrecht, The Netherlands MEMBERS 1. APPENZELLER, Landessternwarte Heidelberg-Konigstuhl, Germany 1. N. BAHCALL, The Institute for Advanced Study, Princeton, U.S.A. P. BERTOLA, Universitd di Padova, Italy J. P. CASSINELLI, University of Wisconsin, Madison, U.S.A. C.1. CESARSKY, Centre d'Etudes de Saclay, Gif-sur-Yvette Cedex, France O. ENGVOLD, Institute of Theoretical Astrophysics, University of Oslo, Norway R. McCRAY, University of Colorado, JlLA, Boulder, U.S.A. P. O. MURDIN, Royal Greenwich Observatory, Cambridge, U.K. F. PACINI, Istituto Astronomia Arcetri, Firenze, Italy V. RADHAKRISHNAN, Raman Research Institute, Bangalore, India K. SATO, School of Science, The University of Tokyo, Japan F. H. SHU, University of California, Berkeley, U.S.A. B. V. SOMOV, Astronomical Institute, Moscow State University, Russia R. A. SUNYAEV, Space Research Institute, Moscow, Russia Y. TANAKA, Institute of Space & Astronautical Science, Kanagawa, Japan S. TREMAINE, CITA, Princeton University, U.S.A. N. O. WEISS, University of Cambridge, U.K. THE DYNAMIC SUN Proceedings of the Summerschool and Workshop held at the Solar Observatory, Kanzelhohe, Austria, Kărnten, August 30-September 10, 1999 edited hy ARNOLD HANSLMEIER Institute for Geophysies, Alfrophysics alU! Meteomlogv, Unh'ersify of Gra::., AIIIlria MAURO MESSEROTII Trie,I'le AHrO/lOmical Ob.\en"alOn, Itah and ASTRlD VERONIG bwifUie for Geophysics, ASlmphysics and Meleorolo/iY, UnivefIity of Gr az, Al/siria SPRINGER SCIENCE+BUSINESS MEDIA, B.V. A C.I.P. CataJogue record for this book is available from the Library of Congress. ISBN 978-94-010-3826-3 ISBN 978-94-010-0760-3 (eBook) DOI 10.1007/978-94-010-0760-3 Printed on acid-free paper Ali Rights Reserved © 2001 Springer Science+Business Media Dordrecht OriginalLy published by Kluwer Academic Publishers in 2001 Softcover reprint of the hardcover 1s t edition 2001 No part of the material protected by this copyright notice may be reproduced or utilized in any form or by any means, electronic or mechanical, inc1uding photocopying, recording or by any information storage and retrieval system, without written permission from the copyright owner. v Table of Contents Pr'eface IX List of Participants xi Invited Lectures Highlights from SOHO and Future Space Missions B. Fleck 1 Solar Instrumentation O. von der Luhe 43 Solar Activity Monitoring M. M esserotti 69 Space Weather and the Earth's Climate N.B. Crosby 95 Solar Magnetohydrodynamics R. W. Walsh 129 The Navier-Stokes Equations and their Solution: Convection and Oscillation Excitation M.P. Rast 155 Solar Polarimetry and Magnetic Field Measurements J. C. del Toro Iniesta 183 Contributed Papers High-Resolution Solar Imaging Using Blind Deconvolution K. Hartkom 211 The Trieste Solar Radio System: A Surveillance Facility for the Solar Corona M. Messerotti, P. Zlobec, M. Comari, C. Dainese, L. Demicheli, L. Fomasari, S. Padovan and L. Perla 215 Deconvolutions and Power Spectra of Solar Granulation K.N. Pikalov and A. Hanslmeier 219 Computational Methods Concerning the Solar Granulation W. Piitzi, A. Hanslmeier and P.N. Brandt 223 Solar Activity Monitoring and Flare Alerting at Kanzelhohe Solar Observatory M. Steinegger', A. Veronig, A. Hanslmeier, M. Messerotti and W. Otruba 227 vi Analytical Modeling of Composed Cylindrical Magnetic Structures in the Corona V.M. Cadei, A. Debosscher, M. Messerotti and P. Zlobec 231 Physical Conditions in Solar Coronal Holes on the Base of Non-LTE Calculations E. Malanushenko and E. Baranovsky 235 X-Ray Limb Flares with Plasma Ejections K. Mikurda, R. Falewicz and P. Pres 239 Coincidences between Magnetic Oscillations and Ha Bright Points P.P. Moretti, A. Cacciani, M. Messerotti, A. Hanslmeier and W. Otruba 243 Chromospheric Dynamics as can be Inferred from Sumer ISOHO Observations J. Rybak, A. Kucera, W. Curdt, U. Schiihle and H. Wohl 247 Formation of Coronal Shock Waves B. Vrsnak 251 Onset of Metric and Kilometric Type II Bursts B. Vrsnak 255 Observations of NOAA 8210 Using MOF and DHC of Kanzelhohe Solar Observatory A. Warmuth, A. Hanslmeier, M. Messerotti, A. Cacciani, P.P. Moretti and W. Otruba 259 On the Rigid Component in the Solar Rotation R. Brajsa, V. Ruidjak, B. Vrsnak, H. Wohl, S. Pohjolainen and S. Urpo 263 The Location of Solar Oscillations in the Photosphere A. Hanslmeier, A. Kucera, .1. Rybak and H. Wohl 267 High Resolution Observations of a Photospheric Light Bridge J. Hirzberger, A. Hanslmeier, J.A. Bonet and M. Vazquez 271 Phases of the 5-min Photospheric Oscillations above Granules and Intergranular Lanes E. V. Khomenko 275 A Photometric and Magnetic Analysis of the Wilson Effect M. Steinegger, .l.A. Bonet, M. Vazquez and V. Martinez Pillet 279 VB Modeling VIRGO Spectral and Bolometric Irradiances with MDI Data M. Steinegger, A. Hanslmeier, W. Otruba, P.N. Brandt, Z. Eker, C. Wehrli and W. Finsterle 283 Generated Langmuir Wave Distribution of an Electron Beam Group C. Estel and G. Mann 287 Magnetoacoustic Surface Waves at the Base of the Convection Zone C. Foullon and B. Roberts 291 Small-Scale Magnetic Elements in 2-D N onstationary Magnetogranulation A.S. Gadun and S.K. Solanki 295 Multi-Mode Kink Instability as a Mechanism for a-Spot Formation M.G. Linton 299 A Numerical Method for Studies of 3D Coronal Field Structures Z. Romeou and T. Neukirch 303 Numerical Modeling of Transition Region Dynamics L. Teriaca and J. G. Doyle 307 The Effect of Azimuthal Magnetic Field on the Magnetostatic Models of Sunspots P.B. Tiwari 311 Comparison of Local and Global Fractal Dimension Determination Methods A. Veronig, A. Hanslmeier and M. Messerotti 315 A uthor Index 319 IX Preface This book contains the proceedings of the Summerschool and Work shop The Dynamic Sun held from August 30th to September 10th, 1999, at the Solar Observatory Kanzelhohe, which belongs to the Institute of Geophysics, Astrophysics and Meteorology of the University of Graz, Austria. This type of conference was the second one held at Kanzelhohe and was again very successful in bringing together experts from specialized topics in solar physics and young scientists and students from different countries. Seven series of lectures were given by invited lecturers, experts in the rele vant fields and twenty-seven contributions were presented at the workshop by the participants. The scientific topics addressed covered a wide range of subjects, from solar magnetohydrodynamics to the physics of the outer solar atmosphere and from a detailed description of the SORO mission to the space weather. The selection of the Kanzelhohe Solar Observatory located in Central Europe, Austria, was quite successful, as, on the one hand, it favored the at tendance of colleagues from the former Eastern countries and, on the other hand, it permitted to present new instrumental developments to the inter national scientific community, such as the installation of a solar monitoring system at Kanzelhohe. On behalf of the organizing committee and all the participants, we wish to thank the following organizations and companies for their financial sup port: The Austrian Bundesministerium fur Wissenschaft und Forschung, Land Karnten, Land Steiermark, European Space Agency (ESA), Markt gemeinde Treffen, University of Graz, Trieste Astronomical Observatory, Ostreicher Company, Creaso Company. We also acknowledge the Univer sity of Trieste and its Department of Astronomy for having accorded their scientific sponsorship to the initiative. Graz, December 2000 Arnold Ranslmeier, Mauro Messerotti and Astrid Veronig Xl List of Participants BAUER Gunter, Graz, Austria ([email protected]) BENSBY Thomas, Lund, Sweden ([email protected]) BOBERG Fredrik, Lund, Sweden ([email protected]) BRAJSA Roman, Zagreb, Croatia ([email protected]) BRUNNER Gerd, Graz, Austria ([email protected]) CROSBY Norma, Noordwijk, The Netherlands ([email protected]) ESTEL Cornelia, Potsdam, Germany ([email protected]) FLECK Bernhard, Greenbelt, USA ([email protected]) FOULLON Claire, St. Andrews, UK ([email protected]) GADUN Aleksey, Kiev, Ukraine ([email protected]) GONZI Siegfried, Graz, Austria ([email protected]) HANSLMEIER Arnold, Graz, Austria ([email protected]) HARTKORN Klaus, Freiburg, Germany ([email protected]) HIRZBERGER Johann, Gottingen, Germany ([email protected]) HUBER Klaus, Graz, Austria, ([email protected]) KHOMENKO Elena, Kiev, Ukraine ([email protected]) KUCERA Ales, Tatranska Lomnica, Slowakia ([email protected]) LINTON Mark, Washington, USA ([email protected]) von der LUHE Oskar, Freiburg, Germany ([email protected]) MALANUSHENKO Elena, Crimea, Ukraine ([email protected]) MESSEROTTI Mauro, Trieste, Italy ([email protected]) MIKURDA Katarzyna, Wroclav, Poland ([email protected]) MORETTI Pier Francesco, Rome, Italy ([email protected]) OTRUBA Wolfgang, Kanzelhohe, Austria ([email protected]) PIKALOV Konstantin, Kiev, Ukraine ([email protected]) POTZI Werner, Graz, Austria ([email protected]) PUSCHMANN Klaus, La Laguna, Spain ([email protected]) RAST Mark P., Boulder, USA ([email protected]) ROMEOU Zaharenia, St. Andrews, UK ([email protected]) RUZDJAK Vladimir, Zagreb, Croatia ([email protected]) RYBAK Jan, Tatranska Lomnica, Slowakia ([email protected]) SANCHEZ CUBERES Monica, La Laguna, Spain ([email protected]) STEINEGGER Michael, Big Bear, USA ([email protected]) TERIACA Luca, Armagh, UK ([email protected]) TIWARI Prithu Bharti, Bangalore, India ([email protected]) del TORO INIESTA Jose Carlos, Granada, Spain ([email protected]) VERONIG Astrid, Graz, Austria ([email protected]) VRSNAK Bojan, Zagreb, Croatia ([email protected]) WALSH Robert, St. Andrews, UK ([email protected]) WARMUTH Alexander, Graz, Austria ([email protected]) HIGHLIGHTS FROM SOHO AND FUTURE SPACE MISSIONS BERNHARD FLECK ESA Space Science Department, NASA/GSFC Mailcode 682.3 Greenbelt, MD 20771, USA ([email protected]) Abstract. The Solar and Reliospheric Observatory (SORO) has provided an unparalleled breadth and depth of information about the Sun, from its interior, through the hot and dynamic atmosphere, out to the solar wind. Analysis of the helioseismology data from SORa has shed new light on a number of structural and dynamic phenomena in the solar interior, such as the absence of differential rotation in the radiative zone, subsurface zonal and meridional flows, sub-convection-zone mixing, a possible circumpolar jet, and very slow polar rotation. Evidence for an upward transfer of mag netic energy from the Sun's surface toward the corona has been established. The ultraviolet instruments have revealed an extremely dynamic solar at mosphere where plasma flows play an important role. Electrons in coronal holes were found to be relatively "cool", whereas heavy ions are extremely hot and have highly anisotropic velocity distributions. The source regions for the high speed solar wind has been identified and the acceleration pro files of both the slow and fast solar wind have been measured. This paper tries to summarize some of the most recent findings from the SORa mission. Present plans for future solar space missions are also briefly discussed. Key words: Sun, Solar Interior, Solar Corona, Solar Wind, SORa 1. Introduction SORO, the Solar and Reliospheric Observatory, is a project of international cooperation between ESA and NASA to study the Sun, from its deep core to the outer corona, and the solar wind (Domingo et al., 1995). It carries a complement of twelve sophisticated instruments, developed and furnished by twelve international PI consortia involving 39 institutes from fifteen countries (Belgium, Denmark, Finland, France, Germany, Ireland, Italy, A. Hanslmeier et al. (eds.). The Dynamic Sun. 1-41. © 2001 Kluwer Academic Publishers.