Hostname: page-component-78c5997874-m6dg7 Total loading time: 0 Render date: 2024-11-19T15:35:23.229Z Has data issue: false hasContentIssue false
  • English
  • Français

Electromagnetic emission by subsequent processes L→L'+S and L+L'→T

Published online by Cambridge University Press:  08 June 2011

Marian Karlický  and
Miroslav Bárta
Marian Karlický
Affiliation:
Astronomical Institute of the Academy of Sciences of the Czech Republic, CZ – 25165 Ondřejov, Czech Republic email: [email protected], [email protected]
Miroslav Bárta
Affiliation:
Astronomical Institute of the Academy of Sciences of the Czech Republic, CZ – 25165 Ondřejov, Czech Republic email: [email protected], [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Using a 2.5-D electromagnetic particle-in-cell (PIC) model, very early stages of a generation of the electromagnetic emission produced by a monochromatic Langmuir wave are studied. It is found that the electromagnetic emission, which is dominant on the harmonic of the plasma frequency, starts to be generated in a very small region of k-vectors. Later on the k-vectors of this emission are scattered around a ‘circle’ (in our 2-D case), given by the relations for the L+L'→T process. Analytical analysis of two subsequent processes L→L'+S a L+L'→T confirms these results.

Keywords

wavesradiation mechanisms: generalSun: radio radiation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S274: Advances in Plasma Astrophysics , September 2010 , pp. 252 - 254
Copyright
Copyright © International Astronomical Union 2011

References

Bárta, M. & Karlický, M. 2000, A&A, 353, 757Google Scholar
Benz, A. O. 1993, Plasma Astrophysics (Kluwer Acad. Publ., Dordrecht, The Netherlands)CrossRefGoogle Scholar
Melrose, D. B. 1980, Plasma Astrophysics (Gordon and Breach Sci. Publ., New York)Google Scholar
Robinson, P. A. 1977, Reviews of Modern Physics, 69, 509Google Scholar
Sakai, J. I. & Nagasuki, Y. 2007, A&A, 474, L33Google Scholar
Willes, A. J., Robinson, P. A., & Melrose, D. B. 1996, Phys. Plasmas, 3 (1), 149CrossRefGoogle Scholar
Yu, H., & Guangli, H. 2008, Adv. Space Res., 41, 1202CrossRefGoogle Scholar