Titlebook: Cosmic Rays, Supernovae and the Interstellar Medium; Maurice M. Shapiro,Rein Silberberg,John P. Wefel Book 1991 Springer Science+Business

Constrain

Stable-Angina

ns will be used to evaluate the upper limit to the number of the black holes in the Galaxy and to fit the γ-ray COS B experimental data of the quasar 3C 273 and to predict the neutrino fluxes from the directions of 3C 273 and the Galactic Center.

雕鏤

支柱

A Brief Introduction to the Cosmic Radiationhing the earth and the “primordial” or source composition; the energy spectra and their modulation in the heliosphere; the effects of magnetic fields, notably on the directional distribution; the propagation of the GCR in the interstellar medium (ISM), and what is inferred about abundances, especial

斑駁

The Composition of the Cosmic Rays: An Updatecceleration and the conditions in the interstellar medium through which the particles travel. Recent (1988–90) measurements and interpretations have provided new information on cosmic ray composition and source abundances. These new results are described and compared to previous work.

FLAX

口訣法

Source Composition, Sites of Origin and Acceleration of Cosmic Raysulations make corrections for the nuclear spallation reactions suffered by the cosmic-ray nuclei in the interstellar gas and clouds. To learn about the sites of origin, the source composition is compared with the general Galactic abundance of elements and isotopes, which is based on spectroscopic st

挑剔為人

Cosmic-Ray Age and the Interstellar Mediumhe galactic gas proves to be very essential for the interpretation of the data on the content of secondary stable and radioactive isotopes in the cosmic rays. Constraints on a galactic wind and on cosmic-ray distributed acceleration in the interstellar medium are discussed.

lactic

The Production of Antiprotons in the Interstellar Gas by Propagating Cosmic Raysof cosmic ray origin and propagation. We have present a detailed discussion of the equilibrium antiprotonproton ratio predictions calculated in the Standard Leaky Box Model and in the diffusive reacceleration model, where cosmic ray particles are reaccelerated due to gyroresonant interaction with hy