Hostname: page-component-77c89778f8-gvh9x Total loading time: 0 Render date: 2024-07-19T16:00:59.143Z Has data issue: false hasContentIssue false
  • English
  • Français

Implications of Observations of the Solar Wind and Corona for Solar Wind Models

Published online by Cambridge University Press:  12 April 2016

W.I. Axford  and
J.F. McKenzie
W.I. Axford
Affiliation:
Max-Planck-Institut fuer Aeronomie, 37191 Katlenburg-Lindau, Germany
J.F. McKenzie
Affiliation:
Max-Planck-Institut fuer Aeronomie, 37191 Katlenburg-Lindau, Germany

Abstract

An abstract is not available for this content so a preview has been provided. As you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
Image of the first page of this content. For PDF version, please use the ‘Save PDF’ preceeding this image.'
Type
Keynote Address
Information
International Astronomical Union Colloquium , Volume 154: Solar and Interplanetary Transients , 1996 , pp. 1 - 3
Copyright
Copyright © Kluwer 1997