TY - JOUR
T1 - Simulation of mode conversion from UHR-mode wave to LO-mode wave in an inhomogeneous plasma with different wave normal angles
AU - Kalaee, Mohammad Javad
AU - Ono, Takayuki
AU - Katoh, Yuto
AU - Iizima, Masahide
AU - Nishimura, Yukitoshi
N1 - Funding Information:
Acknowledgments. The authors would like to express their sincere thanks to both reviewers for the constructive comments and suggestions. The computations were performed by the KDK system of research Institute for Sustainable Humanosphere (RISH) at Kyoto University as a collaborative research project. This work was supported by Tohoku University Global COE program “Global Education and Research Center for Earth and Planetary Dynamics” and by Grant-in-Aid for Scientific Research (21840011) from the Ministry of Education, Culture, Sports, Science and Technology of Japan.
PY - 2009
Y1 - 2009
N2 - We have investigated a linear mode conversion process among UHR-mode, Z-mode, and LO-mode waves by a computer simulation solving Maxwell's equations and the motion of a cold electron fluid. The characteristics of the wave coupling process occurring in the cold magnetized plasma were examined in detail for the case of an inhomogeneity of plasma density lying perpendicular to the ambient magnetic field. The dependence of the conversion efficiency on the incident wave normal angle, wave frequency, background plasma frequency, and steepness of density gradient was studied. The results show that an efficient mode conversion occurred in the conversion process from Z-mode to LO-mode waves rather than from the coupling between UHR-mode to LOmode waves. They also show that the highest conversion efficiency was obtained under the specific condition of the wave normal angle for the incident waves. In the specific case of such critical wave normal angles, we found that perpendicular components of refractive indexes became zero at the site of mode conversion, which is consistent with previously published results. We also show that the range of the critical normal angle varied depending on both the plasma frequency and the wave frequency. The simulation results also reveal that, when the steepness of the density gradient was taken into consideration, efficient mode conversion could be expected even in the case of the mismatch of the refractive indexes preventing the close coupling of plasma waves.
AB - We have investigated a linear mode conversion process among UHR-mode, Z-mode, and LO-mode waves by a computer simulation solving Maxwell's equations and the motion of a cold electron fluid. The characteristics of the wave coupling process occurring in the cold magnetized plasma were examined in detail for the case of an inhomogeneity of plasma density lying perpendicular to the ambient magnetic field. The dependence of the conversion efficiency on the incident wave normal angle, wave frequency, background plasma frequency, and steepness of density gradient was studied. The results show that an efficient mode conversion occurred in the conversion process from Z-mode to LO-mode waves rather than from the coupling between UHR-mode to LOmode waves. They also show that the highest conversion efficiency was obtained under the specific condition of the wave normal angle for the incident waves. In the specific case of such critical wave normal angles, we found that perpendicular components of refractive indexes became zero at the site of mode conversion, which is consistent with previously published results. We also show that the range of the critical normal angle varied depending on both the plasma frequency and the wave frequency. The simulation results also reveal that, when the steepness of the density gradient was taken into consideration, efficient mode conversion could be expected even in the case of the mismatch of the refractive indexes preventing the close coupling of plasma waves.
KW - LO-mode
KW - Mode conversion
KW - Numerical simulation
KW - Wave generation process
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U2 - 10.1186/BF03352977
DO - 10.1186/BF03352977
M3 - Article
AN - SCOPUS:76549129233
SN - 1343-8832
VL - 61
SP - 1243
EP - 1254
JO - Earth, Planets and Space
JF - Earth, Planets and Space
IS - 11
ER -