Skip to main content
Log in

Multi-Site Spectrographic and Heliographic Observations of Radio Fine Structure on April 10, 2001

  • Published:
Solar Physics Aims and scope Submit manuscript

Abstract

We present results of the first simultaneous observations of zebra patterns (ZPs) with super-fine spiky structure in the microwave range made at two observatories ∼1000 km apart (Beijing and Nanjing, China). The fine structure was recorded by a spectra polarimeter in the 5.2 – 7.6 and 2.8 – 3.6 GHz ranges at the Huairou station and by the spectrometer in the 4.5 – 7.5 GHz range at the Purple Mountain Observatory. Simultaneously, the locations of radio sources were observed by the Siberian Solar Radio Telescope (SSRT) at 5.7 GHz. For a general analysis of the April 10, 2001 event, the Solar and Heliospheric Observatory/Michelson Doppler Imager (SOHO/MDI) data and Transition Region and Coronal Explorer (TRACE) images in EUV 171 Å line were used. The circular polarization degree was very weak for the burst background radio emission and moderate to strong for the fine structure. The polarization sign in all the cases probably corresponds to the extraordinary wave mode. Estimations of the magnetic field values in the whistler model for fine structure agree well with the extrapolated values from magnetic maps. Given the possibility of wave transformation in the perpendicular magnetic field and the spiky structure of the ZP, the whistler wave model appears to be the most appropriate explanation for the zebra stripe phenomenon.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Similar content being viewed by others

References

  • Altyntsev, A.T., Kuznetsov, A.A., Meshalkina, N.S., Rudenko, G.V., and Yan, Yihua: 2005, Astron. Astrophys. 431, 1037.

  • Aschwanden, M.J.: 2004, Physics of the Solar Corona, Springer, Praxis Publishers, Chichester, UK.

    Google Scholar 

  • Aschwanden, M.J., Newmark, J.S., Delabouniere, J.-P., et al.: 1999, Astrophys. J. 515, 842.

    Article  ADS  Google Scholar 

  • Benz, A.O.: 1993, Plasma Astrophysics, Kinetic Processes in Solar and Stellar Coronae, Kluwer Academic Publisher, Dordrecht.

    Google Scholar 

  • Chernov, G.P.: 1976, Soviet Astron. 20, 582.

    ADS  Google Scholar 

  • Chernov, G.P.: 1990a, Soviet Astron. 34, 66.

    ADS  Google Scholar 

  • Chernov, G.P.: 1990b, Solar Phys. 130, 75.

    Article  ADS  Google Scholar 

  • Chernov, G.P.: 1996, Astron. Rep. 40, 561.

    ADS  Google Scholar 

  • Chernov, G.P.: 2005, Plasma Phys. Rep. 31, 314.

    Article  ADS  Google Scholar 

  • Chernov, G.P., Yan, Y.H., and Fu, Q.J: 2003, Astron. Astrophys. 406, 1071.

    Article  ADS  Google Scholar 

  • Chernov, G.P., Markeev, A.K., Poquerusse, M., Bougeret, J.L., Klein, K.-L., Mann, G., Aurass, H., and Aschwanden M.J.: 1998, Astron. Astrophys. 334, 314.

    ADS  Google Scholar 

  • Chernov, G.P., Fu, Q.J., Lao, D.B., and Hanaoka, Y.: 2001a, Solar Phys. 201, 153.

    Article  ADS  Google Scholar 

  • Chernov, G.P., Yasnov, L.V., Yan, Y.H., and Fu, Q.J.: 2001b, Chin. J. Astron. Astrophys. 1, 525.

    Article  ADS  Google Scholar 

  • Elgaroy: 1982, Intermediate Drift Bursts, Report 53, ITA, University of Oslo.

  • Fleishman, G.D., Fu, Q.J., Huang, G.L., Melnikov, V.F., and Wang, M.: 2002, Astron. Astrophys. 385, 671.

    Article  ADS  Google Scholar 

  • Foley, C.R., Harra, L.K., Culhane, J.L., and Mason, K.O.: 2001, Astrophys. J. 560, L91.

    Article  ADS  Google Scholar 

  • Fu, Q.J., Qin, J.H., Ji, H.R., and Pei, L.B.: 1995, Solar Phys. 160, 97.

    Article  ADS  Google Scholar 

  • Handy, B.N., Acton, L.W., Kankelborg, C.C., Wolfson, C.J., Akin, D.J., and 43 co-authors: 1999, Solar Phys. 187, 229.

  • Karlicky, M., Barta, M., Jiricka, K., Meszarosova, H., Fernandes, F.C.R., and Cecatto, J.R.: 2001, Astron. Astrophys. 375, 638.

    ADS  Google Scholar 

  • Kruger, A.: 1979, Introduction to Solar Radio Astronomy and Radio Physics, Reidel, Dordrecht.

    Google Scholar 

  • Kuijpers, J.: 1975, Solar Phys. 44, 173.

    Article  ADS  Google Scholar 

  • Kuznetsov, A.A.: 2005, Astron. Astrophys. 438, 341.

    Article  ADS  Google Scholar 

  • LaBelle, J., Treumann, R.A., Yoon, P.H., and Karlicky, M.: 2003, Astrophys. J. 593, 1195.

    Article  ADS  Google Scholar 

  • Maltseva, O.A. and Chernov, G.P.: 1989, Kinematika i Fizika Nebesnykh Tel 5, 39.

    ADS  Google Scholar 

  • Mollwo, L.: 1983, Solar Phys. 83, 305.

    Article  ADS  Google Scholar 

  • Mollwo, L.: 1988, Solar Phys. 116, 323.

    ADS  Google Scholar 

  • Sakurai, T., Ishimoto, K., Nishino, Y., Shinodo, K., and 10 co-authors: 1995, PASJ, 47, 81.

  • Slottje, C.: 1981, Atlas of Fine Structures of Dynamic Spectra of Solar Type IV-dm and Some Type II Radio Bursts, Utrecht Observatory.

  • Winglee, R.M. and Dulk G.A.: 1986, Astrophys. J. 307, 808.

    Article  ADS  Google Scholar 

  • Yan, Y. and Sakurai, T.: 1997, Solar Phys. 174, 65.

    Article  ADS  Google Scholar 

  • Yan, Y. and Sakurai, T.: 2000, Solar Phys. 195, 89.

    Article  ADS  Google Scholar 

  • Zheleznykov, V.V. and Zlotnik, E.Ya.: 1975, Solar. Phys. 44, 461.

    Article  ADS  Google Scholar 

  • Zlotnik, E.Ya., Zaitsev, V.V., Aurass, H., and Hofmann, A.: 2003, Astron. Astrophys. 410, 1011.

    Article  MATH  ADS  Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Corresponding author

Correspondence to G. P. Chernov.

Rights and permissions

Reprints and permissions

About this article

Cite this article

Chernov, G.P., Sych, R.A., Yan, Y. et al. Multi-Site Spectrographic and Heliographic Observations of Radio Fine Structure on April 10, 2001. Sol Phys 237, 397–418 (2006). https://doi.org/10.1007/s11207-006-0111-8

Download citation

  • Received:

  • Accepted:

  • Published:

  • Issue Date:

  • DOI: https://doi.org/10.1007/s11207-006-0111-8

Keywords

Navigation