Skip to main content

Gamma Rays and the Distribution of Cosmic Rays in the Galaxy

  • Chapter
  • 148 Accesses

Part of the book series: NATO ASI Series ((ASIC,volume 210))

Abstract

A brief assessment if given of the question of a gradient of cosmic ray intensity in the Galaxy. It is concluded that there is certainly a gradient in the electron component. Concerning the nuclear component there is less certainty although the present author inclines to the view that there is a gradient here too; certainly a consistent picture can be constructed in which both electrons and nuclei have gradients of magnitude which bear a simple relationship one to the other.

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

Buying options

Chapter
USD   29.95
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
eBook
USD   169.00
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
Softcover Book
USD   219.99
Price excludes VAT (USA)
  • Compact, lightweight edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info
Hardcover Book
USD   219.99
Price excludes VAT (USA)
  • Durable hardcover edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info

Tax calculation will be finalised at checkout

Purchases are for personal use only

Learn about institutional subscriptions

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

References

  • Bloemen, J. B. G. M. 1985, Ph.D. thesis, University of Leiden.

    Google Scholar 

  • Bloemen, J. B. G. M. 1985, Proc. 19th Int. Conf. on Cosmic Rays, 1, 329.

    Google Scholar 

  • Bhat, C. L. Issa, M. R., Mayer, C. J., and Wolfendale, A. W. 1985, Nature, 314, 515.

    Article  ADS  Google Scholar 

  • Bhat, C. L., Mayer, C. J., Rogers, M., Wolfendale, A. W., and Zan, M. 1986, J. Phys., (in press).

    Google Scholar 

  • Dodds, D., Strong, A. W., and Wolfendale, A. W. 1975, Mon. Not. R. Astr. Soc, 171, 569.

    ADS  Google Scholar 

  • Issa, M. R., Riley, P. A., Strong, A. W., and Wolfendale, A. W. 1981, J. Phys., G.7, 565.

    Article  ADS  Google Scholar 

  • Kiraly, P. et al. 1979, Riv. del Nuovo Cimento, 2, 7.

    Google Scholar 

  • Mayer-Hasselwander, H. A. et al. 1982,Astron. and Astrophys., 105, 167.

    ADS  Google Scholar 

  • Morfill, G. E. 1982, Astrophys. J., 262, 749.

    Article  ADS  Google Scholar 

  • Osborne, J. L., Parkinson, M., Richardson, K. M., and Wolfendale, A. W. 1986, previous paper.

    Google Scholar 

  • Riley, P. A., and Wolfendale, A. W. 1984, J. Phys. G.t 19, 1269.

    Article  ADS  Google Scholar 

  • Strong, A. W. 1985,Astron. and Astrophys., 145, 81.

    ADS  Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Editor information

Editors and Affiliations

Rights and permissions

Reprints and permissions

Copyright information

© 1987 D. Reidel Publishing Company

About this chapter

Cite this chapter

Wolfendale, A.W. (1987). Gamma Rays and the Distribution of Cosmic Rays in the Galaxy. In: Morfill, G.E., Scholer, M. (eds) Physical Processes in Interstellar Clouds. NATO ASI Series, vol 210. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-3945-5_7

Download citation

  • DOI: https://doi.org/10.1007/978-94-009-3945-5_7

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-8250-1

  • Online ISBN: 978-94-009-3945-5

  • eBook Packages: Springer Book Archive

Publish with us

Policies and ethics