Hostname: page-component-586b7cd67f-t8hqh Total loading time: 0 Render date: 2024-11-26T00:47:29.387Z Has data issue: false hasContentIssue false
  • English
  • Français

A composite solution of field-line reconnexion

Published online by Cambridge University Press:  13 March 2009

Tyan Yeh
Tyan Yeh
Affiliation:
Pure and Applied Science Division, Global Enterprises, Inc., Louisville, Colorado 80027
Get access Rights & Permissions [Opens in a new window]

Abstract

A solution of the Mhd equations is presented, which describes field-line reconnexion by stagnant diffusion in the middle of a piecewise-uniform convective hydromagnetic flow. This composite solution demonstrates that the diffusion region adjusts its shape and size in accommodation to the incident merging fluids.

Type
Research Article
Information
Journal of Plasma Physics , Volume 14 , Issue 3 , December 1975 , pp. 449 - 453
Copyright
Copyright © Cambridge University Press 1975

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

REFERENCES

Petscheck, H. E. 1964 AAS-NASA Symposium on the Physics of Solar Flares (ed. Hess, W. N.). NASA SP-50, 425.Google Scholar
Sonnerup, B. U. Ö 1970 J. Plasma Phys. 4, 161.CrossRefGoogle Scholar
Sonerup, B. U. Ö 1973 NASA Symposium on High Energy Phenomena on the Sun (ed. Ramaty, R. and Stone, R. G.). NASA SP-342, 357.Google Scholar
Yeh, T. & Axford, W. I. 1970 J. Plasma Phys. 4, 207.CrossRefGoogle Scholar
Yeh, T. & Dryer, M. 1973 Astrophys. J. 182, 301.CrossRefGoogle Scholar