Modification of Karasawa tropospheric scintillation model for Malaysia climate
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Abstract
Tropospheric scintillation is the rapid fluctuation and degradation of satellite signals due to changes in refractive index of atmosphere. This phenomenon tends to affect signals more strongly at frequencies above 10 GHz. This paper introduces a new scintillation prediction model created by modifying the existing Karasawa model. The proposed model is compared with currently existing model using scintillation data collected in Parit Buntar, Malaysia. The proposed model can simultaneously predict scintillation intensity of both fade and enhancement scintillation with an error rate below 5 %.
Keywords
Tropospheric scintillation Ku-band Satellite communicationPACS Nos.
92.60.hf 84.40.UaNotes
Acknowledgments
The authors would like to acknowledge Universiti Kebangsaan Malaysia, the Universiti Sains Malaysia, the MOSTI grant Science Fund (01-01-92-SF0670), the UKM-GGPM-ICT-108-2010, and the Association of Radio Industry Businesses (ARIB) of Japan for providing instruments used to collect data.
References
- [1]F A Semire, R M Mokhtar, W Ismail, N Mohamad and J S Mandeep Adv. Spa. Res. 50 1241 (2012)CrossRefADSGoogle Scholar
- [2]J S Mandeep and M T Islam Adv. Geoph. 60 1180 (2012)ADSGoogle Scholar
- [3]N A Rahim, R Islam, J S Mandeep and H Dao Res. J. App. Sci. Eng. Tech. 4 1616 (2012)Google Scholar
- [4]A Jain, S Tiwari, S Jain and A K Gwal Indian J. Phys. 85 1367 (2011)CrossRefADSGoogle Scholar
- [5]S K Sarkar, M M Gupta and A K De Indian J. Phys. 87 1 (2013)CrossRefADSGoogle Scholar
- [6]A Kumar Indian J. Phys. 87 411 (2013)CrossRefADSGoogle Scholar
- [7]C S Rai Indian J. Phys. 86 709 (2011)CrossRefADSGoogle Scholar
- [8]ITU-R Recommendation ITU-R P 618-9 (2012)Google Scholar
- [9]J S Mandeep Int. J. Phy. Sci. 6 2649 (2011)Google Scholar
- [10]Y Karasawa, M Yarnada and J Allnutt IEEE Trans. on Ant. Prop. 36 1608 (1988)CrossRefADSGoogle Scholar
- [11]I E Otung IEEE Trans. Ant. Prop. 44 1600 (1996)CrossRefADSGoogle Scholar
- [12]S K Midya and U Saha Indian J. Phys. 85 1461 (2011)CrossRefADSGoogle Scholar