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  • © 1998

Polar Cap Boundary Phenomena

Part of the book series: Nato Science Series C: (ASIC, volume 509)

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Table of contents (32 chapters)

  1. Front Matter

    Pages i-xviii
  2. Recent Work on the Kelvin-Helmholtz Instability at the Dayside Magnetopause and Boundary Layer

    • C. J. Farrugia, F. T. Gratton, L. Bender, J. M. Quinn, R. B. Torbert, N. V. Erkaev et al.
    Pages 1-14
  3. Magnetopause Motions in a Newton-Busemann Approach

    • M. P. Freeman, C. J. Farrugia
    Pages 15-26
  4. Comparison of Gasdynamics and MHD Predictions for Magnetosheath Flow

    • N. V. Erkaev, C. J. Farrugia, H. K. Biernat
    Pages 27-40
  5. Time—Varying Reconnection

    • H. K. Biernat, V. S. Semenov, O. A. Drobysh, C. J. Farrugia, N. V. Erkaev
    Pages 41-50
  6. Solar Wind He2+ and H+ Distributions in the Cusp for Southward IMF

    • S. A. Fuselier, E. G. Shelley, W. K. Peterson, O. W. Lennartsson
    Pages 63-72
  7. Open and Closed Low Latitude Boundary Layer

    • Patrick T. Newell, Ching-I. Meng
    Pages 91-101
  8. The Dynamic Magnetosphere

    • T. A. Potemra
    Pages 103-114
  9. Large-Scale Electric Fields in the Dayside Magnetosphere

    • M. I. Pudovkin, A. Egeland
    Pages 141-156
  10. Polar Observations of Cusp Electrodynamics: Evolution from 2- to 4-Cell Convection Patterns

    • N. C. Maynard, W. J. Burke, D. R. Weimer, F. S. Mozer, J. D. Scudder, W. K. Peterson et al.
    Pages 157-172
  11. Relationship between Large-, Meso-, and Small-Scale Field-Aligned Currents and their Current Carriers

    • M. Yamauchi, R. Lundin, L. Eliasson, S. Ohtani, J. H. Clemmons
    Pages 173-188
  12. The Dayside Aurora and its Regulation by the Interplanetary Magnetic Field

    • P. E. Sandholt, C. J. Farrugia, J. Moen, B. Lybekk
    Pages 189-208

About this book

These proceedings are based on the invited talks and selected research reports presented at the NATO Advanced Study Institute (ASI) on "POLAR CAP BOUNDARY PHENOMENA" held at Longyearbyen, Svalbard, June 4 - 13, 1997. The role of the polar cap and its boundary is very substantial in solar-terrestrial physics. At this NATO AS! a major change in thinking on the "cusp" precipitation region in the high-latitude days ide upper atmosphere was reflected, at least for intervals when the interplanetary magnetic field (IMF) is directed southward. It is likely that this has implications for northward IMF as well. The change comes from the now almost complete acceptance of the concept of magnetosheath particle entry along open magnetic field lines and the evolution of the precipitation into the upper atmosphere with time elapsed since magnetic reconnection which opened the field line. A key prediction of this view is that the low-latitude boundary layer (LLBL) is on open field lines.

Editors and Affiliations

  • University Courses on Svalbard, Longyearbyen, Norway

    J. Moen

  • Department of Physics, University of Oslo, Oslo, Norway

    A. Egeland

  • Rutherford Appleton Laboratory, Chilton, UK

    M. Lockwood

Bibliographic Information

Buy it now

Buying options

eBook USD 39.99
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
Softcover Book USD 54.99
Price excludes VAT (USA)
  • Compact, lightweight edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info

Tax calculation will be finalised at checkout

Other ways to access