Convective laser filamentation instability in magnetized plasma

Author:

Bawa’aneh M.S.1,Assayed Ghada2,Said M.R.3,Al-Awfi S.4

Affiliation:

1. Khalifa University of Science Technology and Research, P. O. Box 573, Sharjah, United Arab Emirates.

2. Department of Physics, The Hashemite University, P.O. Box 150459, Zarqa, Jordan.

3. Physics Department, King Faisal University, P.O. Box 400, Al-Ahsa 31982, Kingdom of Saudi Arabia.

4. Department of Physics, Taibah University, Madina, Saudi Arabia.

Abstract

The convective amplification of filamentation instability (FI) of electromagnetic waves traveling along the density ramp of a magnetized plasma is investigated. The generalized amplification factor of the instability in the presence of a DC–magnetic field is derived by obtaining the governing equations of the instability and using the slow-coupling technique to obtain an analytical expression for the amplification factor in weakly magnetized plasma. The result shows enhancement of the convective FI gain by the magnetic field, where the enhancement is stronger for lower equilibrium plasma density values.

Publisher

Canadian Science Publishing

Subject

General Physics and Astronomy

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