Skip to main content
Log in

Magnetopause magnetic barrier parameters in dependence on the solar wind magnetic field orientation

  • Published:
Annales Geophysicae

Abstract

Some theories predict the magnetosheath magnetic field strength will decrease and the density increase just outside the dayside magnetopause as the interplanetary magnetic field turns southward. Two studies have recently reported results which confirm these expectations. In contrast, we briefly review our own theoretical predictions which indicate that precisely the opposite effect is expected. We survey new and previously reported magnetosheath observations and demonstrate that they are consistent with the predictions of our model. The conflicting results indicate a need for further theoretical and observational work.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Subscribe and save

Springer+ Basic
$34.99 /Month
  • Get 10 units per month
  • Download Article/Chapter or eBook
  • 1 Unit = 1 Article or 1 Chapter
  • Cancel anytime
Subscribe now

Buy Now

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Similar content being viewed by others

Author information

Authors and Affiliations

Authors

About this article

Cite this article

Pudovkin, M.I., Zaitseva, S.A. & Besser, B.P. Magnetopause magnetic barrier parameters in dependence on the solar wind magnetic field orientation. Annales Geophysicae 13, 828–835 (1995). https://doi.org/10.1007/s00585-995-0828-y

Download citation

  • Received:

  • Revised:

  • Accepted:

  • Issue Date:

  • DOI: https://doi.org/10.1007/s00585-995-0828-y

Keywords

Navigation