Solar Physics

, Volume 153, Issue 1, pp 73–89

Material ejection

  • D. F. Webb
  • T. G. Forbes
  • H. Aurass
  • J. Chen
  • P. Martens
  • B. Rompolt
  • V. Rušin
  • S. F. Martin
Article

DOI: 10.1007/BF00712493

Cite this article as:
Webb, D.F., Forbes, T.G., Aurass, H. et al. Sol Phys (1994) 153: 73. doi:10.1007/BF00712493

Abstract

This paper reviews the major discussions and conclusions of the Flares 22 Workshop concerning the physical processes involved in mass ejecta events, with an emphasis on large-scale phenomena, especially Coronal Mass Ejections (CMEs). New insights have been gained from recent data obtained from the SMM andYohkoh spacecraft and from several new ground-based radio and optical instruments, as well as from theoretical advances concerning the origins, driving mechanisms and long-term evolution of CMEs.

Copyright information

© Kluwer Academic Publishers 1994

Authors and Affiliations

  • D. F. Webb
    • 1
  • T. G. Forbes
    • 2
  • H. Aurass
    • 3
  • J. Chen
    • 4
  • P. Martens
    • 5
  • B. Rompolt
    • 6
  • V. Rušin
    • 7
  • S. F. Martin
    • 8
  1. 1.Institute for Space Research, Boston CollegeNewton CenterUSA
  2. 2.Space Science Center/EOS, Morse HallUniversity of New HampshireDurhamUSA
  3. 3.Astrophysical Institute, PotsdamObs. f. Solare RadioastronomieTremsdorfGermany
  4. 4.Code 6790, Beam Physics BranchNaval Research LaboratoryWashington, D.C.USA
  5. 5.ESTEC/ESASpace Science DivisionAG NoordwijkThe Netherlands
  6. 6.Astronomical Institute of Wroclaw UniversityWroclawPoland
  7. 7.Astronomical InstituteSlovak Academy of SciencesTatranská LomnicaSlovakia
  8. 8.Solar Astronomy 264-33California Institute of TechnologyPasadenaUSA