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Coronal Holes and Solar Wind Acceleration

Proceeding of the SOHO-7 Workshop, held at Asticou Inn in Northeast Harbor, Maine, U.S.A., from 28 September–1 October, 1998

  • John L. Kohl
  • Steven R. Cranmer

Table of contents

  1. Front Matter
    Pages i-xi
  2. Introductory and Summary Presentations

  3. Working Group Presentations

    1. Jean-Loup Bertaux, Erkki Kyrölä, Eric Quemerais, Rosine Lallement, Walter Schmidt, Tuula Summanen et al.
      Pages 129-132
    2. Rita Betta, Salvatore Orlando, Giovanni Peres, Salvatore Serio
      Pages 133-136
    3. F. Chiuderi-Drago, A. Kerdraon, E. Landi, A. Fludra
      Pages 141-144
    4. I. Cuseri, D. Mullan, G. Poletto
      Pages 153-156
    5. R. B. Dahlburg, G. Einaudi
      Pages 157-160
    6. I. E. Dammasch, D. M. Hassler, W. Curdt, K. Wilhelm
      Pages 161-164
    7. D. Dobrzycka, L. Strachan, M. P. Miralles, J. L. Kohl, L. D. Gardner, P. Smith et al.
      Pages 177-180
    8. D. A. Falconer, R. L. Moore, J. G. Porter, D. H. Hathaway
      Pages 181-184
    9. A. Fludra, G. Del Zanna, B. J. I. Bromage
      Pages 185-188
    10. R. A. Frazin, A. Ciaravella, E. Dennis, S. Fineschi, L. D. Gardner, J. Michels et al.
      Pages 189-192
    11. C. P. T. Groth, D. L. De Zeeuw, T. I. Gombosi, K. G. Powell
      Pages 193-198
    12. M. Guhathakurta, E. C. Sittler, D. McComas
      Pages 199-206
    13. P. Hackenberg, G. Mann, E. Marsch
      Pages 207-210
    14. B. Inhester, G. Stenborg, R. Schwenn, N. Srivastava, B. Podlipnik
      Pages 211-214
    15. Margarita Karovska, Brian E. Wood, John W. Cook, Russell A. Howard, Guenter E. Brueckner
      Pages 219-222
    16. R. Keppens, J. P. Goedbloed
      Pages 223-226
    17. J. L. Kohl, S. Fineschi, R. Esser, A. Ciaravella, S. R. Cranmer, L. D. Gardner et al.
      Pages 233-236
    18. M. Kojima, K. Fujiki, T. Ohmi, M. Tokumaru, A. Yokobe, K. Hakamada
      Pages 237-239
    19. E. Landi, H. E. Mason, M. Landini
      Pages 241-244
    20. M. Landini, A. Brković, E. Landi, I. Rüedi, S. Solanki
      Pages 245-248
    21. P. Lemaire, K. Bocchialini, V. Aletti, D. Hassler, K. Wilhelm
      Pages 249-252
    22. Xing Li
      Pages 253-256
    23. L. Maccari, G. Noci, S. Fineschi, A. Modigliani, M. Romoli, J. L. Kohl
      Pages 265-268
    24. W. H. Matthaeus, G. P. Zank, R. J. Leamon, C. W. Smith, D. J. Mullan, S. Oughton
      Pages 269-275
    25. Mari Paz Miralles, L. Strachan, L. D. Gardner, P. L. Smith, J. L. Kohl, M. Guhathakurta et al.
      Pages 277-281
    26. R. L. Moore, D. A. Falconer, J. G. Porter, S. T. Suess
      Pages 283-286
    27. L. Ofman, M. Romoli, G. Noci, G. Poletto, J. L. Kohl, R. A. Howard et al.
      Pages 287-290
    28. S. Patsourakos, J.-C. Vial, J.-R. Gabryl, S. Koutchmy, U. Schühle
      Pages 291-294
    29. S. Poedts, A. D. Rogava, S. M. Mahajan
      Pages 295-298
    30. U. Schühle, W. Curdt, K. Wilhelm, S. K. Solanki, K. Stucki
      Pages 299-302

About this book

Introduction

The SOHO-7 Workshop was held from 28 September through 1 October 1998 at the Asticou Inn in Northeast Harbor, Maine. The primary topic of this Workshop was the impact of SOHO observations on our understanding of the nature and evolution of coronal holes and the acceleration and composition of the solar wind. The presentations and discussions occasionally went beyond this topic to include the impact of the reported research on other solar structures and the heliosphere. SOHO (the Solar and Heliospheric Observatory), a project of international cooperation between ESA and NASA, was launched in December 1995 and began its science operations during the first few months of 1996. To many solar and space physicists, it was a great advantage that SOHO began itscomprehensive look at the Sun during the 1996 solar minimum. The qualitatively simple two-phase corona, with polar coronal holes expanding into the high-speed solar wind, and a steady equatorial streamer belt related somehow to the stochastic slow-speed solar wind, allowed various SOHO diagnostics to be initiated with a reasonably well­ understoodcircumsolar geometry. The analysis of subsequentSOHO measurements made during the rising phase of solar cycle 23 will continue to benefit from what has been learned from the first two years of data.

Keywords

Corona Planet Solar wind Variation solar

Editors and affiliations

  • John L. Kohl
    • 1
  • Steven R. Cranmer
    • 1
  1. 1.Harvard-Smithsonian Center for AstrophysicsCambridgeUSA

Bibliographic information

  • DOI https://doi.org/10.1007/978-94-015-9167-6
  • Copyright Information Springer Science+Business Media B.V. 1999
  • Publisher Name Springer, Dordrecht
  • eBook Packages Springer Book Archive
  • Print ISBN 978-90-481-5267-4
  • Online ISBN 978-94-015-9167-6
  • Buy this book on publisher's site
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