Magnetic field observations of the jovian magnetosphere suggest an extended magnetic tail, which has been formed by solar wind interaction with the planetary field.
This is a preview of subscription content, access via your institution
Access options
Subscribe to this journal
Receive 51 print issues and online access
$199.00 per year
only $3.90 per issue
Buy this article
- Purchase on Springer Link
- Instant access to full article PDF
Prices may be subject to local taxes which are calculated during checkout
References
Van Allen, J. A. et al. Science 188, 459–462 (1974).
Smith, E. J. et al. J. geophys. Res. 79, 3501–3513, 1974.
Goertz, C. K. Space Sci. Rev. 23, 319–344 (1979).
Northrop, T. G., Goertz, C. K. & Thomsen, M. F. J. geophys. Res. 79, 3579–3583 (1974).
Kivelson, M. G., Coleman, P. J., Froidevanx, L. & Rosenberg, R. L. J. geophys. Res. 83, 4823–4841, 1978.
Smith, E. J., Davis, L. Jr & Jones, D. E. Jupiter (ed. Gehrels, T. 788–829 (University of Arizona Press, 1976).
Dessler, A. J. & Vasyliunas, V. Geophys. Res. Lett. 6, 37–40 (1979).
Acuna, M. & Ness, N. F. J. geophys. Res. 81, 2917–2922 (1976).
Ness, N. F. et al. Science 204, 982–987 (1979).
Ness, N. F. J. geophys. Res. 70, 2989–3005 (1965).
Ness, N. F., Behannon, K. W., Lepping, R. P. & Whang, Y. C. J. geophys. Res. 80, 2708–2716, 1975.
Carr, T. D. & Desch, M. D. in Jupiter (ed. Gehrels, T.) 693–737 (University of Arizona Press, 1976).
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Ness, N., Acuna, M., Lepping, R. et al. Jupiter's magnetic tail. Nature 280, 799–802 (1979). https://doi.org/10.1038/280799a0
Received:
Accepted:
Issue Date:
DOI: https://doi.org/10.1038/280799a0