Results 191 to 200 of about 163,915 (242)
Increased and varied radiation during the Sun's encounters with cold clouds in the last 10 million years. [PDF]
Opher M +9 more
europepmc +1 more source
Chemical Environment and Temperature Effects on the Formation and Destruction of C<sub>3</sub>O<sub>2</sub> in Cosmic-Ray-Processed Ices. [PDF]
Pilling S +3 more
europepmc +1 more source
Particle background characterization and prediction for the NUCLEUS reactor CE ν NS experiment. [PDF]
Abele H +59 more
europepmc +1 more source
A cosmic-ray loaded nascent outflow driven by a massive star cluster. [PDF]
Lemoine-Goumard M +8 more
europepmc +1 more source
Recent production rates of cosmogenic nuclides in the igneous rocks of Jezero crater floor, Mars. [PDF]
Zorzano M- +2 more
europepmc +1 more source
Swift Heavy Ion-Induced Chemistry of CH<sub>3</sub>CN Ices at 10 and 80 K. [PDF]
de Barros ALF +10 more
europepmc +1 more source
Some of the next articles are maybe not open access.
Related searches:
Related searches:
Cosmic γ rays and cosmic-ray particles
Nature, 1983Recent experiments using extensive air shower techniques1–5 have given evidence for the presence of significant fluxes of cosmic γ rays, in the energy range 1015–1016 eV, from specific cosmic sources. We argue here that the flux from these sources, and others as yet unresolved, is probably sufficient to allow the explanation of a number of previously ...
J. Wdowczyk, A. W. Wolfendale
openaire +3 more sources
Chemical Society Reviews, 2013
Gas-phase chemistry in the interstellar medium is driven by fast ion-molecule reactions. This, of course, demands a mechanism for ionization, and cosmic rays are the ideal candidate as they can operate throughout the majority of both diffuse and dense interstellar clouds.
Nick, Indriolo, Benjamin J, McCall
openaire +2 more sources
Gas-phase chemistry in the interstellar medium is driven by fast ion-molecule reactions. This, of course, demands a mechanism for ionization, and cosmic rays are the ideal candidate as they can operate throughout the majority of both diffuse and dense interstellar clouds.
Nick, Indriolo, Benjamin J, McCall
openaire +2 more sources
Space Science Reviews, 1998
Secondary radioactive isotopes that are used for the determination of cosmic-ray age have relatively short decay lifetimes. The measured abundance of these isotopes at low energies is representative of the cosmic-ray diffusion and the gas distribution in a region of a few hundred parsecs around the Sun.
Vladimir S. Ptuskin, Aimé Soutoul
openaire +1 more source
Secondary radioactive isotopes that are used for the determination of cosmic-ray age have relatively short decay lifetimes. The measured abundance of these isotopes at low energies is representative of the cosmic-ray diffusion and the gas distribution in a region of a few hundred parsecs around the Sun.
Vladimir S. Ptuskin, Aimé Soutoul
openaire +1 more source

