Catalog of Solar Particle Events 1955–1969

Prepared under the Auspices of Working Group 2 of the Inter-Union Commission on Solar-Terrestrial Physics

  • H. W. Dodson
  • E. R. Hedeman
  • R. W. Kreplin
  • M. J. Martres
  • V. N. Obridko
  • M. A. Shea
  • D. F. Smart
  • H. Tanaka
  • Z. Švestka
  • P. Simon

Part of the Astrophysics and Space Science Library book series (ASSL, volume 49)

Table of contents

  1. Front Matter
    Pages I-IX
  2. H. W. Dodson, E. R. Hedeman, R. W. Kreplin, M. J. Martres, V. N. Obridko, M. A. Shea et al.
    Pages 1-23
  3. H. W. Dodson, E. R. Hedeman, R. W. Kreplin, M. J. Martres, V. N. Obridko, M. A. Shea et al.
    Pages 25-142
  4. H. W. Dodson, E. R. Hedeman, R. W. Kreplin, M. J. Martres, V. N. Obridko, M. A. Shea et al.
    Pages 143-242
  5. H. W. Dodson, E. R. Hedeman, R. W. Kreplin, M. J. Martres, V. N. Obridko, M. A. Shea et al.
    Pages 243-410
  6. Back Matter
    Pages 411-430

About this book

Introduction

This Catalog originated as a common enterprise of solar physicists and space scientists under the auspices of the Second Working Group of the Inter-Union Commission of Solar Terrestrial Physics (IUCSTP). It is a pleasure to acknowledge the support we received from the IUCSTP president, Dr H. Friedman, and the IUCSTPSecretary, Dr E. R. Dyer during the several years we have spent on this project. The aim of our work has been to assemble all observations of particle events from the first PCA observation in 1955 through two solar cycle maxima up to the end of 1969, in order to preserve these data from the first epoch of the space era in a concise form for use in the future. Because the techniques of observation have very much improved in the present solar cycle, there is a tendency to consider the observations before 1964 as incomplete and out-of-date; one must not forget, however, that the 19th solar cycle greatly differed from cycle No. 20 in the level of its activity, and also may have been the last cycle of strong activity for many decades to come. Therefore, the particle event observations before 1964 'should be compiled in a consistent manner for comparison with later observations, and we believe that the Catalog achieves this. The rapid development of the exploration techniques necessarily results in a significant amount of inhomogeneity in the Catalog, as increasingly smaller events were detected.

Keywords

energy physics solar

Authors and affiliations

  • H. W. Dodson
    • 1
  • E. R. Hedeman
    • 1
  • R. W. Kreplin
    • 2
  • M. J. Martres
    • 3
  • V. N. Obridko
    • 4
  • M. A. Shea
    • 5
  • D. F. Smart
    • 5
  • H. Tanaka
    • 6
  1. 1.The McMath-Hulbert Observatory of the University of MichiganPontiacUSA
  2. 2.The Naval Research LaboratoryUSA
  3. 3.Observatoire de ParisMeudonFrance
  4. 4.IZMIRANMoscowUSSR
  5. 5.Air Force Cambridge Research LaboratoriesBedfordUSA
  6. 6.Research Institute of AtmosphericsToyokawaJapan

Editors and affiliations

  • Z. Švestka
    • 1
    • 2
  • P. Simon
    • 3
  1. 1.Fraunhofer InstituteFreiburg im BreisgauGermany
  2. 2.American Science and EngineeringCambridgeUSA
  3. 3.Observatoire de ParisMeudonFrance

Bibliographic information

  • DOI https://doi.org/10.1007/978-94-010-1742-8
  • Copyright Information Springer Science+Business Media B.V. 1975
  • Publisher Name Springer, Dordrecht
  • eBook Packages Springer Book Archive
  • Print ISBN 978-94-010-1744-2
  • Online ISBN 978-94-010-1742-8
  • Series Print ISSN 0067-0057
  • About this book