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Fan and horseshoe instabilities -relation to the low frequency waves registered by Cluster in the polar cusp

Fan and horseshoe instabilities -relation to the low frequency waves registered by Cluster in the polar cusp . J .B łę cki (1) , M.Parrot ( 2 ), S.Savin ( 3 ), R.Wronowski (1) , N.Cornilleau-Wehrlin ( 4 ), E. Amata (5). (1) Space Research Centre PAS 00-716 Warsaw, Bartycka 18A, Poland,

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Fan and horseshoe instabilities -relation to the low frequency waves registered by Cluster in the polar cusp

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  1. Fan and horseshoe instabilities -relation to the low frequency waves registered by Cluster in the polar cusp J.Błęcki (1),M.Parrot (2), S.Savin(3),R.Wronowski(1), N.Cornilleau-Wehrlin(4), E. Amata (5). (1) Space Research Centre PAS 00-716 Warsaw, Bartycka 18A, Poland, (4) LPCE/CNRS, Orléans, France (3) Space Research Institute RAS, Moscow, Russia (4) CETP/Velizy, France (5) IFSI/INAF, Rome, Italy XVII CLUSTER Workshop, Uppsala, 14 May 2009

  2. Main modes of the plasma waves in the cusp XVII CLUSTER Workshop, Uppsala, 14 May 2009

  3. Magion4 observations in the polar cusp Blecki et al. ASR, 1997 XVII CLUSTER Workshop, Uppsala, 14 May 2009

  4. 04:03:36 UT Savin et al. 2004 XVII CLUSTER Workshop, Uppsala, 14 May 2009

  5. XVII CLUSTER Workshop, Uppsala, 14 May 2009

  6. Fan Instability • First studies by Kadomtsev and Pogutse (1967), discussed in relation to auroral region by Omelchenko et al. (JGR 1994) and Vaivads et al. (1997), solar wind and auroral region by Krafft and Volokitin (2003and 2004) and magnetopause by Savin (2004). • Fan instability is driven by a particle beam along the magnetic field lines but in contrast to the usual beam-plasma instabilities it does not require a threshold in the relative velocity and positive slope in the distribution function • Long superthermal tail in the distribution function is needed for developing of this instability • The electron tail that forms drives the anomalous Dopplerresonance instability–which results in pitch angle scattering of the electrons and the generation of cyclotron radiation. XVII CLUSTER Workshop, Uppsala, 14 May 2009

  7. Electrostatic aproximation Vaivads et al.. 1997 Kraft and Volokitin 2003 extended the model on so-called electromagnetic lower hybrid waves They applied their model to study emissions in solar wind,where The same condition is applicable for the polar cusp It gives dispersion relation Kraft and Volokitin 2003 XVII CLUSTER Workshop, Uppsala, 14 May 2009

  8. For auroral magnetosphere they obtained Next paper by Kraft and Volokitin 2004 brings the nonlinear analysis of the wave – particle and wave-wave interactions. They shown importance of these processes for the lower hybrid branch of electromagnetic waves XVII CLUSTER Workshop, Uppsala, 14 May 2009

  9. XVII CLUSTER Workshop, Uppsala, 14 May 2009

  10. For polar cusp one can assume simplification • Frequency • Oblique propagation • Maximum of the spectral density for 0.2<cosΘ<0.4 • For the outer cusp • 0.19ωce<ω<0.38 ωce XVII CLUSTER Workshop, Uppsala, 14 May 2009

  11. Fan instability 13.03.2003 XVII CLUSTER Workshop, Uppsala, 14 May 2009

  12. XVII CLUSTER Workshop, Uppsala, 14 May 2009

  13. XVII CLUSTER Workshop, Uppsala, 14 May 2009

  14. XVII CLUSTER Workshop, Uppsala, 14 May 2009

  15. XVII CLUSTER Workshop, Uppsala, 14 May 2009

  16. Plasmawavesinthe polar cuspatthe ionospheric altitude - registrations by DEMETER DEMETER is a low-altitude satellite (710 km) launched in June 2004 onto a polar and circular orbit which measures electromagnetic waves all around the Earth except in the auroral zones (Parrot, 2006). In December 2005, the altitude of the satellite was decreased to 660 km. The ELF/VLF range for the electric field is from DC up to 20 kHz. There are two scientific modes: a survey mode where spectra of one electric and one magnetic component are onboard computed up to 20 kHz and a burst mode where, in addition to the onboard computed spectra, waveforms of one electric and one magnetic field component are recorded up to 20 kHz. The burst mode allows performing a spectral analysis with higher time and frequency resolution. During the burst mode, the waveforms of the six components of the electromagnetic field are also recorded up to 1.25 kHz. This allows performing a detailed wave propagation analysis . XVII CLUSTER Workshop, Uppsala, 14 May 2009

  17. XVII CLUSTER Workshop, Uppsala, 14 May 2009

  18. Polar cusp at the ionospheric level XVII CLUSTER Workshop, Uppsala, 14 May 2009

  19. Kilometric continuum emission cone corotates with plasmasphere mergring with the AKR emission cone on the night side No AKR cusp source found !!!! Green 2003 XVII CLUSTER Workshop, Uppsala, 14 May 2009

  20. 10.03.2006 KR XVII CLUSTER Workshop, Uppsala, 14 May 2009

  21. XVII CLUSTER Workshop, Uppsala, 14 May 2009

  22. SUMMARY and CONCLUSIONS • Broad emissions as the typical feature of the cusp, but characteristic emissions around electron cyclotro frequency • Localized fluxes of energetic electrons and sources of the waves below electron cyclotron frequency • Subtle structure of the sources • Fan instability as an effective source of the waves below electron gyrofrequency • Lower hybrid waves as a accelerator of particles • Measurements at the ionospheric altitude (~700km) done by DEMETER show presence of the energetic electrons together with low frequency waves. • Presence of the kilometric radiation at the boundary of the cusp together with energetic electron fluxes XVII CLUSTER Workshop, Uppsala, 14 May 2009

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