Abstract
Much of the magnetic field in solar and stellar photospheres is arranged into clusters of “flux tubes”, i.e., clustered into compact areas in which the intrinsic field strength is approximately a kilogauss. The flux concentrations are constantly evolving as they merge with or annihilate against other concentrations, or fragment into smaller concentrations. These processes result in the formation of concentrations containing widely different fluxes. Schrijver et al (1997, Paper I) developed a statistical model for this distribution of fluxes, and tested it on data for the quiet Sun. In this paper we apply that model to a magnetic plage with an average absolute flux density that is 25 times higher than that of the quiet network studied in Paper I. The model result matches the observed distribution for the plage region quite accurately. The model parameter that determines the functional form of the distribution is the ratio of the fragmentation and collision parameters. We conclude that this ratio is the same in the magnetic plage and in quiet network. We discuss the implications of mis for (near-)surface convection, and the applicability of the model to stars other than the Sun and as input to the study of coronal heating.
This is a preview of subscription content, log in via an institution.
Buying options
Tax calculation will be finalised at checkout
Purchases are for personal use only
Learn about institutional subscriptionsPreview
Unable to display preview. Download preview PDF.
References
Hagenaar, H. J., Schrijver, C.J., and Title, A. M.: 1997, Astrophys. J., in preparation.
Martin, S. F., Livi, S. H. B., and Wang, J.: 1955, Australian J. Phys. 38, 929.
Parker, E. N.: 1994, Spontaneous Current Sheets in Magnetic Fields, Oxford Uinversity Press, Oxford.
Priest, E, R., Parnell, C. E., and Martin, S.F.: 1994, Astrophys. J. 427, 459.
Ryutova, M. P., Kaisig, M., and Tajima, T.; 1996, Astrophys. J. 459, 744.
Scherrer, P. H., Bogart, R. S., Bush, R. I., Hoeksema, J. T., Kosovichev, A. G., Schou, J., Rosenberg, W., Springer, L., Tarbell, T. D., Title, A., Wolfson, C. J., Zayer, I., and The MDI Engineering Team: 1995, Solar Phys. 162, 129.
Schrijver, C. J.: 1987, Astron. Astrophys. 180, 241.
Schrijver, C. I: 1993, Astron. Astrophys. 269, 395.
Schrijver, C. J. and Harvey, K. L.: 1989, Astrophys. J. 343, 481.
Schrijver, C. J. and Martin, S. F.: 1990, Solar Phys. 129, 95.
Schrijver, C. J., Zwaan, C., Balke, A. C., Tarbell, T. D., and Lawrence, J. K.: 1992, Astron. Astrophys. 253, L1.
Schrijver, C. J., Shine, R. A., Hagenaar, H. J., Hurlburt, N. E., Title, A. M., Strous, L. H., Jefferies, S. M., Jones, A. R., Harvey, J. W., and Duvall, Th. L: 1996, Astrophys. J. 468, 921.
Schrijver, C. J., Title, A. M., van Ballegooijen, A. A., Hagenaar, H. J., and Shine, R. A.: 1997, Astrophys. J. in press.
Spruit, H. C., Nordlund, Å, and Title, A. M.: 1990, Ann. Rev. Astron. Astrophys. 28, 263.
Wang, Y.-M. and Sheeley N. R., Jr.: 1991, Astrophys. J. 375, 761.
Wang, Y.-M. and Sheeley, N. R., Jr.: 1994, Astrophys. J. 430, 399.
Zwaan, C.: 1978, Solar Phys, 60, 213.
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1997 Springer Science+Business Media Dordrecht
About this chapter
Cite this chapter
Schrijver, C.J., Title, A.M., Hagenaar, H.J., Shine, R.A. (1997). Modeling the Distribution of Magnetic Fluxes in Field Concentrations in a Solar Active Region. In: Fleck, B., Švestka, Z. (eds) The First Results from SOHO. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-5236-5_18
Download citation
DOI: https://doi.org/10.1007/978-94-011-5236-5_18
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-6204-6
Online ISBN: 978-94-011-5236-5
eBook Packages: Springer Book Archive