Hostname: page-component-78c5997874-ndw9j Total loading time: 0 Render date: 2024-11-04T18:37:07.919Z Has data issue: false hasContentIssue false
  • English
  • Français

Observational Tests of a Double Loop Model for Solar Flares

Published online by Cambridge University Press:  05 March 2013

S. J. Hardy ,
D. B. Melrose  and
H. S. Hudson
S. J. Hardy
Affiliation:
Research Centre for Theoretical Astrophysics, School of Physics, University of Sydney, NSW 2006, Australia; [email protected]
D. B. Melrose
Affiliation:
Research Centre for Theoretical Astrophysics, School of Physics, University of Sydney, NSW 2006, Australia; [email protected]
H. S. Hudson
Affiliation:
Solar Physics Research Corp., 4720 Calle Desecada, Tucson, AZ 85718, USA ISAS, 3–1-1 Yoshinodai, Sagamihara, Kanagawa 229, Japan; [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

A model for the energetics of solar flares, developed by Melrose (1997), is based on magnetic reconnection between two current-carrying magnetic loops. A detailed numerical investigation of the model has been made to identify those configurations that lead to energy release in a flare. Our results predict a strong relation between the ratio of currents in the interacting loops for a favoured flare configuration, and provide further support for a proposed method of generating long loops connecting different active regions. Both of these predictions are amenable to observational verification.

Keywords

Sun: flaresmagnetic reconnectionmagnetic flux loops
Type
Research Article
Information
Publications of the Astronomical Society of Australia , Volume 15 , Issue 3 , 1998 , pp. 318 - 324
Copyright
Copyright © Astronomical Society of Australia 1998

References

Hanaoka, Y. 1997, Solar Phys., 173, 319 CrossRefGoogle Scholar
Heyvaerts, J., Priest, E. R., & Rust, D. M. 1977, ApJ, 216, 123 Google Scholar
Machado, M. E., Moore, R. L., Hernandez, A. M., Rovira, M. G., Hagyard, M. J., & Smith, J. B. Jr 1988, ApJ, 326, 425 Google Scholar
Melrose, D. B. 1997, ApJ, 486, 521 (M97)Google Scholar
Nishio, M., Yaji, K., Kosugi, T., Nakajima, H., & Sakurai, T. 1997, ApJ, 489, 976 Google Scholar