Abstract
During the February 3 – 15, 1986 activity complex the region NOAA 4713 is 100 % effective in producing type II burst related flares. It is proposed to explain this fact by the immediate neighborhood of this active region and a non — polar coronal hole with its open magnetic-topology. Synoptic plots of magnetograms illuminate the formation of this rare configuration.
References
Chernov, G.P.: 1988, personal communication.
Garcia, H. A., and Dryer, M.: 1987,Solar Phys. 109, 119.
Gopalswamy, N. and Kundu, M. R.: 1987,Solar Phys.,111, 347.
Harvey, J. W. and Sheeley, N. R., Jr.: 1979,Space Sci. Rev. 23, 139.
Hewish, A.: 1988,Solar Phys. 116, 195.
Künzel, H.: 1962,Astron. Nachr. 286. 6, 267.
Nelson, G. J. and Melrose, D. B.: 1985, in McLean, D. J. and Labrum, N. R. (Eds.),Solar Radiophysics, Cambridge Univ. Press, Cambridge, Great. Britain.
Stewart, R. T.: 1934,Solar Phys. 94, 379.
Solar Geophysical Datas: 1986, No. s499,500,501, Part I; No.504, Part II, U.S. Deptm. of Commerce, Boulder, Colorado, U.S.A.
Švestka, Z.: 1976,Solar Flares, Reidel, Dordrecht, Holland.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Aurass, H., Rendtel, J. Flare — type II — burst association in the February 1986 activity complex. Sol Phys 122, 381–384 (1989). https://doi.org/10.1007/BF00913003
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00913003