Details

IS LINEAR GYRO-RESONANT INTERACTION RESPONSIBLE FOR 2HZ. SIDE BANDS?

Anil Kumar

Department of Physics, PDM College of Engineering, Bahadurgarh (Jhajjar), Haryana -124507 (India).

D.P. Singh

Department of Physics, PPIMT, Chaudharywas (Hisar), Haryana -125001 (India).

Ashwani Kumar

Department of Physics, TRA Memorial Institute of Engg& Technology Mandi (H.P.)-175008.

23-31

Vol: 4, Issue: 2, 2014

Receiving Date: 2014-02-13 Acceptance Date:

2014-04-14

Publication Date:

2014-04-15

Download PDF

Abstract

Wave-particle interaction plays an important role in the morphology of ionosphere and magnetosphere and wave propagation. Common view is that Nonlinear cyclotron interaction between resonant electrons, in resonance with transmitted signals in the magnetosphere in 1-30 kHz range is a reason to cause side bands. Side band spacing of 20 Hz (and above) can easily be explained through nonlinear amplification process. Wave magnetic amplitude of 3-5 pT for wave-particle interaction to occur in the magnetosphere the need for non-linear interaction as per the established theory of Inan (1977). It is shown that wave magnetic amplitude (Bw) only of ~2pTisneeded to cause small-such as 2- 3 Hz side band spacing, which is below 3 pT suggesting that linear gyro-resonant interaction may also be a cause of small side bands.

Keywords: Wave-particle interaction, Trapped particles, VLF Emissions

References

  1. A L Brinca, JGeophys Res(USA),77, (1972) 3508.
  2. CG Park, JGeophysRes (USA), 86,(1981) 2286.
  3. CG Park & DCD Chang, Geophys Res Lett(USA),5,(1978) 861.
  4. DP Singh, Indian J Radio Space, 20, 424, (1991)
  5. DP Singh, Indian J Radio Space, 21, 25,(1992).
  6. DP Singh &UP Singh, Indian J Radio Space Phys , 35, 22, (2006).
  7. DP Singh, UP Singh & RP Singh, Earth,Moon& Planets(The Netherlands) 64 ,145,(1994).
  8. D A McPherson,H C Koons, M H Dazey, R L Dowden, L E S Amon & N R Thomson, Nature,
  9. D A McPherson,H C Koons, M H Dazey, R L Dowden, L E S Amon & N R Thomson, JGeophys Res (USA),79, (1974b) 1555.
  10. H C Koons, M H, Dazey R L Dowden & L E S Amon,J Geophys Res(USA),81,(1976)5536.
  11. J J Angerami & JO Thomas, The distribution of ions and electrons in the earth’s exosphere, Technical Report No. 3412-3, Stanford University, California 1963.
  12. J M Albert, J Geophys Res (USA), 10521191(2000).
  13. M Ikeda M, Indian J Radio Space Phys, 31, (2002) 121.
  14. N Cornilleau-Wehrlin& R Gendrin , J Geophy Res(USA), 84,1979(1979).
  15. R Raghuram , TF Bell &RA Helliwell , Geophys Res Lett(USA), 4, 199(1977).
  16. R.B Horne, R M Thorne,S A Glauert,J M Albert,N P Meredith & R R Anderson , J Geophys Res(USA), 110 A03225 (2005).
  17. R L, Dowden, A D McKay, L E S Amon, H C Koons&MH,Dazey ,J GeophysRes(USA) 83,169(1978).
  18. R L Dowden, Planet & Space Sci(UK), 19,374,(1971).
  19. U S Inan, Non-linear gyroresonant interactions of energetic particles and coherent VLF waves in the magnetosphere, Tech Report No. 3414-3, Stanford Univ, Stanford, California, 1977.
  20. U S Inan, T F Bell &R A Helliwell, J GeophysRes(USA),83,(1978) 3235.
  21. W B Gail, U S Inan, R A Helliwell, &D L Carpenter,,J Geophys Res(USA), 95, 15103(1990).
  22. Ya I Likhter, O A Molchanov&Chymrev,SovPhys JETP(USSR),14,(1971) 325.
Back

Disclaimer: All papers published in IJRST will be indexed on Google Search Engine as per their policy.

We are one of the best in the field of watches and we take care of the needs of our customers and produce replica watches of very good quality as per their demands.