Acceleration of high-energy cosmic rays by pulsars.
High energy cosmic ray origin and acceleration by LF electromagnetic radiation produced by pulsars, noting maximum energy for protons
Gunn, J. E.↗
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Search indexed NASA NTRS and DOE OSTI research on propulsion, heat transfer, battery materials and energy systems. Follow report and document links to the original sources.
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Stochastic variations of cosmic rays in the solar system.
Cosmic ray intensity short term stochastic variations in solar system related to turbulent solar wind day-to-day variations
Jokipii, J. R.↗
Cosmic rays in the Galaxy.
Galactic cosmic rays, discussing chemical composition, isotopic separation, proton and alpha particles energy spectra, propagation, interactions, etc
Meyer, P.↗
Mn-53 and the age of galactic cosmic rays
Mean age of galactic cosmic rays technique based on manganese isotope half life passing through interstellar hydrogen
Reames, D. V.↗
The survival of heavy nuclei in Colgate's supernova-acceleration model for cosmic rays
Heavy nuclei survival in cosmic rays Colgate supernova acceleration model, assuming plasma wave instability in shock wave
Kinsey, J. H.↗
On the convection, diffusion, and adiabatic deceleration of cosmic rays in the solar wind
Cosmic ray transport in solar wind generalized with anisotropic diffusion approximation
Jokipii, J. R.↗
A large area high resolution cosmic ray charge composition detector
Primary cosmic rays balloon-borne charge composition detector in 3-30 Z range
Balasubrahmanyan, V. K.↗
Radial gradients and anisotropies of cosmic rays in the interplanetary medium
Cosmic ray radial gradients and anisotropies, describing behavior in interplanetary medium
Axford, W. I.↗
The propagation of very heavy primary cosmic ray particles
Very heavy primary cosmic ray particles propagation calculation, using fragmentation parameters
Friedlander, M. W.↗
Energy loss of cosmic rays in the interplanetary medium
Cosmic ray energy loss in interplanetary medium, discussing solar wind effects on low energy particles
Fisk, L. A.↗
Silicon burning and the synthesis of cosmic- ray nuclei
Source abundances of cosmic ray nuclei from silicon burning process in supernovae
Reames, D. V.↗
Transport of cosmic rays in the solar corona
Cosmic ray particle transport in solar corona by drifting along current sheets separating discontinuous magnetic field structures
Fisk, L. A.↗
Experiment on S57 (later OSO 3) satellite (cosmic ray charge and energy spectra)
Cosmic ray charge and energy spectra from OSO-3 experiments with details of detector design and operation
Kaplon, M. F.↗
Some characteristics of microwave type 4 radio bursts and the acceleration of solar cosmic rays
Acceleration processes of solar cosmic ray bursts, and microwave type 4 bursts
Sakurai, K.↗
Propagation of cosmic rays in the solar wind
Cosmic rays propagation in solar wind, presenting statistical theory of interplanetary magnetic field effect on charged particles transport
Jokipii, J. R.↗
Convective transport of low energy cosmic rays in the interplanetary region
Cosmic ray propagation in interplanetary space, deriving steady state transport equation with energy losses
Gleeson, L. J.↗
Ultra-heavy cosmic rays in the moon
Ultraheavy cosmic ray nuclei existence inferred from Apollo 12 lunar rock pigeonite crystal track length distribution
Price, P. B.↗
Electron calibration of a high energy cosmic ray detector
The spectrum of cosmic ray electrons above 10 GeV was studied extensively. The spectrum is predicted to steepen at an energy which is related to the lifetime of electrons in the interstellar medium against losses due to inverse Compton collisions with photons and to synchrotron radiation in galactic magnetic fields. The experimental results diverge widely; the lack of agreement between the various measurements is due to a variety of experimental problems.
Simnett, G. M.↗