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Regular and seasonal behaviour of atmospheric radio noise field strength (ARNFS) over low latitude station calcutta

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Summary

The electromagnetic radiation of cloud discharge known as atmospheric radio noise field strength (ARNFS) shows a gradual fall from a frequency of 9 kHz to 81 kHz as studied over a period of two years at Calcutta, very close to Bay of Bengal. The main characteristic features of ARNFS at Calcutta are that-(i) ARNFS shows that midday median value is smaller than midnight median value in all months, (ii) level of daily minimum is higher in February and monsoon compared to other seasons, (iii) ‘sunrise effect’ and ‘sunset effect’ are well correlated with local sunrise and sunset times, (iv) the magnitude of ‘sunrise fade’ and ‘sunrise fade rate’ are maximum in April and lowest during winter period, (v) the magnitude of sunset fade is higher in premonsoon and postmonsoon while it is lowest in monsoon, (vi) number of occurrence of both sunrise effect and sunset effect is remark-ably smaller in monsoon. The positions of the sun and of atmospheric sources are jointly the causes of seasonal and diurnal variations. The missing of ‘sunrise effect’ and ‘sunset effect’ are due to local cloud activity and variation of electron density during geomagnetic storms.

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References

  • Berger, K., 1978: Blitzstrom-Parameter von Aufwärtsblitzen.Bull. Schweiz. Elektrotech. Ver.,69, 353–360.

    Google Scholar 

  • Cowley, S. W. S., Morelli, J. P., Lockwood, M., 1991: Dependence of convective flows and particle precipitation in the high latitude dayside ionosphre on the X and Y components of the interplanetary magnetic field.J. Geophys. Res. 96, 5557–5564.

    Google Scholar 

  • De, B. K., Sakar, S. K., 1986: Effect of geomagnetic storms on sunrise fade of long distance 40 kHz propagation.Meteorol. Atmos. Phys.,35, 227–235.

    Google Scholar 

  • Friedel, R. H. W., Hughes, A. R. W., Dowden, R. L., Adams, C. D. D., 1993: First observations on Trimpi events at Durban (L=1.69) using a OMSKI receiver.J. Geophys. Res.,98, 1571–1580.

    Google Scholar 

  • Hara, T., Horiai, K., 1979: Geomagnetic disturbances and associated phase anomalies of VLF radio wave at middle latitudes.J. Geomagn. Geoelectr.,31, 75–85.

    Google Scholar 

  • Hayakaya, M., Shimakura, S., 1978: On the mechanism of reflection of ELF-LF radio waves from lower ionosphere.Trans. IECE Japan,E61, 15–18.

    Google Scholar 

  • King, J. W., Fooks, L., 1968: Long lasting storm effect in the ionospheric D region.J. Atmos. Terrest. Phys.,30, 639–643.

    Google Scholar 

  • Sarkar, S., Bhattacharya, A. B., Sen, A. K., 1980: On the seasonal variation of VLF atmospherics and rainfall over Calcutta.Ann. Geophys. 80, 67–72.

    Google Scholar 

  • Satori, G., 1991: Combined ionospheric effect due to Forbush decrease and magnetospheric high energy particles at mid latitudes.J. Atmos. Terr. Phys.,53, 325–332.

    Google Scholar 

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De, B.K., Sarkar, S.K. Regular and seasonal behaviour of atmospheric radio noise field strength (ARNFS) over low latitude station calcutta. Meteorl. Atmos. Phys. 61, 107–114 (1996). https://doi.org/10.1007/BF01029715

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  • DOI: https://doi.org/10.1007/BF01029715

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