Published 1988 | Version v1
Miscellaneous Metadata-only

Cosmic ray spectrum produced by supernova remnants with an upper limit on wave dissipation

Creators

Description

By taking into account an upper limit to the wave dissipation we have shown that, within the limitations of test particle theory, supernova remnants (SNR) remain the prime candidates for the interstellar cosmic ray population below 1014 to 1015 eV/n. (orig.)

Additional details

Additional titles

Original title (German)
Das durch Supernova-Ueberreste erzeugte Spektrum der kosmischen Strahlung unter Beruecksichtigung einer oberen Grenze fuer die Wellen-Dissipation

Publishing Information

Imprint Title
Max-Planck-Institute for Nuclear Physics. Annual report 1987
Imprint Pagination
202 p.
Journal Page Range
p. 149.
Report number
INIS-mf--12013

INIS

Country of Publication
Germany
Country of Input or Organization
Germany
INIS RN
21004618
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
DISSIPATION FACTOR; ENERGY SPECTRA; LIMITING VALUES; NONLINEAR PROBLEMS; PRIMARY COSMIC RADIATION; SHOCK WAVES; SUPERNOVA REMNANTS; TEV RANGE 100-1000; WAVE PROPAGATION
Descriptors DEC
COSMIC RADIATION; COSMIC RADIO SOURCES; ENERGY RANGE; IONIZING RADIATIONS; RADIATIONS; SPECTRA; TEV RANGE

Optional Information

Notes
Imprint:Max-Planck-Institut fuer Kernphysik. Jahresbericht 1987.