Acceleration of cosmic rays at the solar-wind boundary.
Acceleration of cosmic rays at solar wind boundaries by outward moving magnetic irregularities
Jokipii, J. R.↗
Engineering topics
Jokipii, J. R.
Publications and source records attributed to Jokipii, J. R..
Backscatter and diffusion of cosmic rays in a random magnetic field.
Backscatter and diffusion for fast cosmic ray charged particles in random magnetic field
Jokipii, J. R.↗
Modulation of low-rigidity cosmic rays and the power spectrum of the interplanetary magnetic field in 1962 and 1965.
Low rigidity cosmic ray modulation and interplanetary medium at solar minimum and at other phases of solar cycle
Jokipii, J. R.↗
Storage and diffusion of cosmic-ray electrons in the galaxy.
Storage, diffusion and energy loss of cosmic ray electron propagation in galaxy, discussing leakage lifetime inadequacies and electron acceleration
Jokipii, J. R.↗
Correlation of greater than or approximately equal to 30-kev electron pulses and magnetic fields in the magnetosheath and beyond.
Electron pulses and magnetic fields in magnetosheath and beyond bow shock studied for correlation by IMP 1 satellite
Jokipii, J. R.↗
Diurnal intensity variation of low-energy electrons observed near the polar cap.
Electron flux and energy spectrum measurements near polar cap investigated for diurnal intensity variations
ELECTRON FLUX↗
Energy changes of cosmic rays in the solar system.
Energy changes between solar wind and cosmic rays, discussing particle motion description by Fokker- Planck differential equation
DIFFERENTIAL EQUATION↗
Solar modulation and the energy density of galactic cosmic rays.
Interstellar gas dynamics suggests that energy density of galactic cosmic rays places firm upper limit on undetermined constant of solar modulation
SOLAR COSMIC RAY↗
Cosmic-ray propagation. I.
Charged particle motion in random magnetic field, describing time evolution of particle distribution in pitch angle and position in terms of Fokker- Planck coefficients
INTERPLANETARY MAGNETIC FIELD↗
Spectral shifts in quasi-stellar objects.
Red shifts and blue shifts relative frequency distribution for QSO
FREQUENCY DISTRIBUTION↗
Pitch-angle dependence of first-order Fermi acceleration at shock fronts.
Pitch-angle dependence of first-order Fermi acceleration of particles trapped between shock front and moving magnetic mirror
PARTICLE ACCELERATION↗
Low-energy cosmic-ray modulation related to observed interplanetary magnetic field irregularities.
Low energy cosmic ray modulation relationship to observed interplanetary magnetic field irregularities in terms of diffusion, using space probes
ENERGY SPECTRUM↗
Diffusion and convection of energetic electrons behind the earth's bow shock.
Energy spectrum change of group of electrons being convected downwind in magnetosheath and behind Earth bow shock
SOLAR WIND↗
A model of Fermi acceleration at shock fronts with an application to the earth's bow shock.
Model of Fermi acceleration at shock front developed and applied to Earth bow shock
BOW SHOCK↗
Spectral shifts in quasi-stellar objects
Red and blue shift frequency distribution of quasi-stellar objects from nearby galaxies
RED SHIFT↗
The spectral shifts of an ensemble of relativistic emitters
Doppler shift toward red found for radiation from ensemble of relativistically moving emitter
DOPPLER EFFECT↗
Effects of diffusion on the composition of the solar corona and the solar wind
Effects of radial diffusion in solar corona and solar wind
CORONA↗
Diffusion and convection of energetic electrons behind the earth's bow shock
Diffusion effects on energy spectrum of electron group analyzed during downwind convection in bow shock transition region of earth
ELECTRON ENERGY↗