Abstract
Observations of cosmic rays and their related radio to gamma-ray signatures are surveyed and discussed critically, and compared to theoretical models of the cosmic-ray origin and propagation. The analogous heliospheric processes are included as a well-studied case of the principal physical processes of energetic particle acceleration and propagation. Reinforcements, or conflicts, in the interpretations of cosmic-ray spectral and compositional characteristics arise when cosmic-ray source and propagation models are confronted with astronomical information about the Galaxy as a whole and from potential source sites, i.e., supernova remnants or regions with high massive-star density. This volume represents the outcome of two workshops held at ISSI. In this chapter we summarize the introductory papers presented below, and include insights from the workshop discussions.
Keywords
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.
This is a preview of subscription content, log in via an institution.
Buying options
Tax calculation will be finalised at checkout
Purchases are for personal use only
Learn about institutional subscriptionsPreview
Unable to display preview. Download preview PDF.
References
Anders, E. and Grevesse, N.: 1989, ‘Abundances of the Elements–Meteoritic and Solar’, Geochim. Cosmochim. Acta 53, 197–214.
Balogh, A., Gosling, J. T., Jokipii, J. R., Kallenbach, R., and Kunow, H. (eds.): 1999, Co-rotating Interaction Regions, Kluwer Academic Publishers, Dordrecht.
Bamert, K., Wimmer-Schweingruber, R. F., Kallenbach, R., Hilchenbach, M., Klecker, B., Bogdanov, A., and Wurz, P.: 2001, ‘Origin of the May 1998 Suprathermal Particles: Results from CELIAS/(H)STOF on board SOHO’, J. Geophys. Res. (submitted).
Boldt, E. and Loewenstein, M.: 2000, ‘Cosmic Ray Generation by Quasar Remnants: Constraints and Implications’, Monthly Notices Roy. Astron. Soc. 316, L29–L33.
Chupp, E. L.: 1990, ‘Transient Particle Acceleration Associated with Solar Flares’, Science 250, 229. Ellison, D. C., Möbius, E., and Paschmann, G.: 1990, ‘Particle Injection and Acceleration in Oblique
Shocks: Comparison of Upstream and Downstream Events’, Astrophys. J. 352, 376–394. Ensslin, T. A., Simon, P., Biermann, P. L., Klein, U., Kohle, S., Kronberg, P. P., and Mack, K.-
H.: 2001, ‘Signatures in a Giant Radio Galaxy of a Cosmological Shock Wave at Intersecting Filaments of Galaxies’, Astrophys. J. 549, L39–L42.
Ferrière, K.: 1998, ‘Global Model of the Interstellar Medium in Our Galaxy with New Constraints on the Hot Gas Component’, Astrophys. J. 497, 759–776.
Fisk, L. A., Kozlovsky, B., and Ramaty, R.: 1974, ‘An Interpretation of the Observed Oxygen and Nitrogen Enhancements in Low-Energy Cosmic Rays’, Astrophys. J. 190, L35.
Fletcher, A. and Shukurov, A.: 1999, in: M. Ostrowski and R. Schlickeiser (eds.), Plasma Turbulence and Energetic Particles in Astrophysics,Krakow, pp. 98–102.
Gallant, Y. A. and Achterberg, A.: 1999, ‘Ultra-high-energy Cosmic Ray Acceleration by Relativistic Blast Waves’, Monthly Notices Roy. Astron. Soc. 305, L6.
Gloeckler, G. and Geiss, J.: 1998, ‘Interstellar and Inner Source Pickup Ions Observed with SWICS on ULYSSES’, Space Sci. Rev. 86, 127–159.
Greisen, K.: 1966, Phys. Rev. Lett. 16, 748.
Jokipii, J. R. and Morfill, G. E.: 1985, ‘On the Origin of High-energy Cosmic Rays’, Astrophys. J. 290, L1 – L4.
Koyama, K., Petre, R., Gotthelf, E. V., Hwang, U., Matsura, M., Ozaki, M., and Holt, S. S.: 1995, ‘Evidence for Shock Acceleration of High-energy Electrons in the Supernova Remnant SN1006’, Nature 378, 255–258.
Meyer, J.-P., Drury, L., and Ellison, D.: 1997, ‘Galactic Cosmic Rays from Supernovae Remnants — I. A Cosmic-Ray Composition Controlled by Volatility and Mass-to-Charge Ratio’, Astrophys. J. 487, 182–196.
Ostrowski, M.: 1998, ‘Acceleration of Ultra-high Energy Cosmic Ray Particles in Relativistic Jets in Extragalactic Radio Sources’, Astron. Astrophys. 335, 134–144.
Parker, E. N.: 1966, ‘The Dynamical State of the Interstellar Gas and Field I’, Astrophys. J. 145, 811–833.
Parker, E. N.: 1967, ‘The Dynamical State of the Interstellar Gas and Field II-III’, Astrophys. J. 149, 517–552.
Parker, E. N.: 1992, ‘Fast Dynamos, Cosmic Rays, and the Galactic Magnetic Field’, Astrophys. J. 401, 137–145.
Pelletier, G. and Kersalé, E.: 2000, ‘Acceleration of UHE Cosmic Rays in Gamma-ray Bursts’, Astron. Astrophys. 361, 788–794.
Pesses, M. E., Eichler, D., and Jokipii, J. R.: 1981, ‘Cosmic Ray Drift, Shock Wave Acceleration, and the Anomalous Component of Cosmic Rays’, Astrophys. J. 246, L85 — L88.
Reynolds, S. P. and Keohane, J. W.: 1999, ‘Maximum Energies of Shock-accelerated Electrons in Young Shell Supernova Remnants’, Astrophys. J. 525, 368–374.
Sorrell, W. H.: 1987, ‘Origin and Acceleration of 1020 eV Cosmic-ray Protons’, Astrophys. J. 323, 647–656.
Terasawa, T. et al.: 1999, ‘Observation of a ‘Cosmic-Ray Modified’ Interplanetary Shock’, Proc. 26th Int. Cosmic Ray Conf., Salt Lake City 6, 528.
Uchihori, Y. et al.: 2000, Astropart. Phys. 13 151.
Vietri, M.: 1995, ‘The Acceleration of Ultra—High-Energy Cosmic Rays in Gamma-Ray Bursts’, Astrophys. J. 453, 883–889.
Wilson, A. S., Young, A. J., and Shopbell, P. L.: 2001, ‘Chandra X-Ray Observations of Pictor A: High-Energy Cosmic Rays in a Radio Galaxy’, Astrophys. J. 547, 740–753.
Zatsepin, G. T. and Kuzmin, V. A.: 1966, JETP Lett. 4, 78.
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 2001 Springer Science+Business Media Dordrecht
About this paper
Cite this paper
Diehl, R., Kallenbach, R., Parizot, E., Von Steiger, R. (2001). The Astrophysics of Galactic Cosmic Rays. In: Diehl, R., Parizot, E., Kallenbach, R., Von Steiger, R. (eds) The Astrophysics of Galactic Cosmic Rays. Space Sciences Series of ISSI, vol 13. Springer, Dordrecht. https://doi.org/10.1007/978-94-017-3239-0_1
Download citation
DOI: https://doi.org/10.1007/978-94-017-3239-0_1
Publisher Name: Springer, Dordrecht
Print ISBN: 978-90-481-5862-1
Online ISBN: 978-94-017-3239-0
eBook Packages: Springer Book Archive