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Recent Progress in Understanding Energy Conversion and Particle Acceleration in the Solar Corona

  • Bernhard Kliem
  • Alec MacKinnon
  • Gérard Trottet
  • Tim Bastian
Part of the Lecture Notes in Physics book series (LNP, volume 612)

Abstract

We report on results of the working group sessions at the CESRA 2001 workshop on “Energy Conversion and Particle Acceleration in the Solar Corona” which was focused on radio observations and related modeling. Progress reached in the following areas is summarized: (1) diagnostics of coronal magnetic fields and the morphology of the field in flares and filament eruptions; (2) evidence of magnetic reconnection and MHD turbulence in radio emissions; (3) acceleration site, propagation, and trapping of radio-emitting energetic particles in flares; (4) the sites of particle acceleration in long duration events, as evidenced by the 2000 July 14 (“Bastille Day”) flare; (5) radio imaging of CMEs and filament eruptions; (6) the relationship of coronal and interplanetary shock waves to flares, CMEs, and other coronal waves; and (7) the origin of solar energetic particles.

Keywords

Solar Phys Magnetic Reconnection Radio Burst Solar Energetic Particle Event Ramaty High Energy Solar Spectroscopic Imager 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer-Verlag Berlin Heidelberg 2003

Authors and Affiliations

  • Bernhard Kliem
    • 1
  • Alec MacKinnon
    • 2
  • Gérard Trottet
    • 3
  • Tim Bastian
    • 4
  1. 1.Astrophysikalisches Institut PotsdamPotsdamGermany
  2. 2.Department of Adult and Continuing EducationUniversity of GlasgowGlasgowUK
  3. 3.LESIA, Observatoire de ParisSection d’Astrophysique de MeudonMeudon-CedexFrance
  4. 4.National Radio Astronomy ObservatoryCharlottesvilleUSA

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