A Back-Tracing Code to Study the Magnetosphere Transmission Function for Primary Cosmic Rays

  1. Tuija I. Pulkkinen,
  2. Nikolai A. Tsyganenko and
  3. Reiner H.W. Friedel
  1. Pavol Bobik1,
  2. Matteo Boschini3,
  3. Davide Grandi3,
  4. Massimo Gervasi4,
  5. Elisabetta Micelotta3 and
  6. Pier-Giorgio Rancoita3

Published Online: 18 MAR 2013

DOI: 10.1029/155GM32

The Inner Magnetosphere: Physics and Modeling

The Inner Magnetosphere: Physics and Modeling

How to Cite

Bobik, P., Boschini, M., Grandi, D., Gervasi, M., Micelotta, E. and Rancoita, P.-G. (2005) A Back-Tracing Code to Study the Magnetosphere Transmission Function for Primary Cosmic Rays, in The Inner Magnetosphere: Physics and Modeling (eds T. I. Pulkkinen, N. A. Tsyganenko and R. H.W. Friedel), American Geophysical Union, Washington, D. C.. doi: 10.1029/155GM32

Author Information

  1. 1

    Institute of Experimental Physics, Kosice, Slovak Republic

  2. 3

    Infn Sezione di Milano, Milano, Italy

  3. 4

    Universitá di Milano-Bicocca, Milano, Italy

Publication History

  1. Published Online: 18 MAR 2013
  2. Published Print: 1 JAN 2005

ISBN Information

Print ISBN: 9780875904207

Online ISBN: 9781118666098

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Keywords:

  • Magnetospheric physics—Simulation methods

Summary

This chapter contains sections titled:

  • Introduction

  • The Transmission Function

  • Primary Particles' Spectra

  • Conclusions