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ИЗМЕНЕНИЯ МАГНИТНОЙ СПИРАЛЬНОСТИ В СОЛНЕЧНОМ ЦИКЛЕ

ИЗМЕНЕНИЯ МАГНИТНОЙ СПИРАЛЬНОСТИ В СОЛНЕЧНОМ ЦИКЛЕ. Kirill Kuzanyan ИЗМИРАН, Россия Zhang H., Gao Yu Национальные Астрономические Обсерватории АН КНР. Question:. Can we learn more of solar activity looking at magnetic helicity?. Dynamo model with evolution of Helicity.

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ИЗМЕНЕНИЯ МАГНИТНОЙ СПИРАЛЬНОСТИ В СОЛНЕЧНОМ ЦИКЛЕ

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  1. ИЗМЕНЕНИЯ МАГНИТНОЙ СПИРАЛЬНОСТИ В СОЛНЕЧНОМ ЦИКЛЕ Kirill Kuzanyan ИЗМИРАН, Россия Zhang H., Gao Yu Национальные Астрономические Обсерватории АН КНР

  2. Question: Can we learn more of solar activity looking at magnetic helicity?

  3. Dynamo model with evolution of Helicity Magnetic field generation (Parker Dynamo) Generation of Helicity Parameterized equation

  4. 20 years systematic monitoring of the solar vector magnetic fields in active regions taken at Huairou Solar observing station, China (1987-2006) More observations from Mitaka (Japan) and also Mees, MSFC (USA) etc., but only Huairou data systematically cover 20 years period.

  5. So, theory requires the mirror asymmetry to be the same from cycle to cycle!How to measure it ?

  6. observations Observable !

  7. Photospheric vector magnetogram of AR 10930 (SOT at Hinode);2006 Dec 11-12 at 23:10:06-00:13:17UT.

  8. AR 10930: HC over the filtergram; positive/negative: a typical AR. The filtergram of AR 10930; contours of current helicity HC for positive (negative) values shown in red (green), corresponding to absolute values of 0.2, 0.5, 1.0, 4.0 G2/m, respectively. The field of view is 104''80''.

  9. Observations and Data Reduction • 983 active regions; 6630 vector magnetograms observed at Huairou Solar Observing Station; • Time ranges from 1988 to 2005; • Time average: 2 year data bins; • Latitudinal: Northern hemisphere and Southern hemisphere (7 degree bins);

  10. Helicity overlaid with butterfly diagram

  11. Force free factor overlaid with butterfly diagram

  12. Compare: Qualitatively, the both quantities are distributed in a similar manner. So, despite the noisy nature of the data, accuracy of measurements is reliable.

  13. THE MAIN RESULT • Current helicity and twist follow the propagation of the magnetic activity dynamo waves recorded by sunspots. The mirror asymmetry plays an important role in the solar dynamo mechanism.

  14. Observable properties of helicity • Anti-symmetric over the solar equator • Cyclic variation 11 years (not 22 years!) • Time lag with respect to sunspots is about 2 years ahead , not behind! (confront with dynamo theory) • Systematic sign inversion of helicity (a) at the beginning of the cycle (b) at the end of the cycle

  15. Simple self-consistent dynamo model with evolution of helicity (dynamical nonlinear dynamo) Kleeorin, Kuzanyan, Moss, Sokoloff, Rogazhevsky, Zhang, A&A, 2003; and a series of publications of the authors thereafter in 2005-2009

  16. Choice of Parameter Range (Example) C=0.01- ok! HELICITY C=0.1 too high value LATITUDE

  17. FURTHER PLAN • Include meridional circulation in order to see its effect on • latitudinal extent of helicity versus sunspots and • the time lag between helicity and sunspots

  18. Kleeorin et al. 2003EVOLUTION OF HELICITY WITH TIME(Northern HemisphereN) S N HELICITY Sunspot Group Number Magnetic Energy ~1988 ~1997 Diffusion Time Units

  19. Summary • Helicity helps in development of self-consistent dynamo models!

  20. Thank you!

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