Document Type : Original Article
Authors
1 Nuclear Science and Technology Research Institute (NSTRI), Tehran, Iran
2 Physics and Energy Engineering Department, Amirkabir University of Technology, Tehran
3 Plasma Technology Research Core, Faculty of Sciences, University of Mazandaran, Babolsar, Iran
4 Department of Marine and Atmospheric Science (Non-Biologic), University of Hormozgan, Bandar Abbas, Iran
Abstract
In this paper the heating effects was investigated with SAMI2 model. An external Gaussian heating source was considered in electron temperature equation that models the radio frequency heating. The effects of the heating were investigated as a function of the heating period, intensity of the heating source, height of the heating center and different latitude of the heating in Iran coordinates. Results of the simulations show that height of the heating and intensity of the source have main role in the distribution function of the electron density and temperature. This distribution in heating zone and conjugate point was shown. In early time of heating, by increasing the height, the electron temperature was increased dramatically. At low intensity of the heating source, the electron temperature wasn’t increased. However, the electron temperature was increased in heating zone after 30 minutes. Also, the heating distributes the electron density counter which represents the reduction of the electron density and the formation of the duct in heating zone and the growth of the electron density at conjugate point. The results show that at low latitude, electron temperature at heating zone and conjugate point was increased more.
Keywords
- D J Gorney, Geophys 28 (1990) 315.
- J M Forbes, S Bruinsma, and F G Lemoine, Science 312 (2006) 1366.
- U S Inan, T F Bell, and J V Rodriguez, Geophys Res. Lett. 18 (1991) 705.
- A P Nickolaenko and M Hayakawa, Geophys Res. Lett. 22 (1995)3015.
- Y B Yao, et all., Chin Sci. Bull. 57 (2012) 500.
- T Yu, et al., Chin Sci. Bull. 54 (2009) 1080.
- T Mao, et al., Chin Sci. Bull. 55 (2010) 712.
- J Lastovicka, Atmos. Solar. Ter.r Phys. 68 (2006) 479.
- J Lastovicka, Space Res. 43 (2009) 1.
- M Mendillo and J M Forbes, Geophys Res. 83 (1978) 151.
- G M Milikh, et al., Geophys Res. Lett. 35 (2008)
- L M Duncan, J P Sheerin, and R A Benke, Rev. Lett. 61, 2 (1988) 239.
- V V Vas’kov, et al., Aeron. 32, 5 (1992) 698.
- J D Huba, G Joyce, and J A Fedder, Res. Lett. 27, 19 (2000b) 3181.
- S W Willis and J R Davis, Geophys. Res. 78 (1973) 5710.
- M M Shoucri, G J Morales, and J E Maggs, Geophys. Res. 89 (1984) 2907.
- R P Perrine, et al., Radio Sci. 41 (2006) RS4002.
- T W Wu, et al., Geophys. Res. Lett. 39 (2012) L07103.