The acceleration of energetic particle fluxes in shock fronts in interplanetary space.
Enhanced fluxes of energetic particles coincident with onset of solar flare initiated Forbush decrease cause particle acceleration in shock wave
Bukata, R. P.↗
Engineering topics
Mccracken, K. G.
Publications and source records attributed to Mccracken, K. G..
Microburst phenomena. I - Auroral-zone X rays.
Auroral zone X ray microbursts with rapid risetimes
Edwards, P. J.↗
Microburst phenomena. II - Auroral-zone electrons.
Auroral zone electron microbursts observed with Injun 3 satellite, discussing time profiles and relation to X ray microbursts
Mccracken, K. G.↗
A comparison of the characteristics of corotating and flare-initiated Forbush decreases.
Flare initiated and corotating Forbush decreases from Pioneer 6 and 7 deep space probes
Bukata, R. P.↗
Cosmic rays - Asymptotic directions, etc.
Asymptotic directions of cosmic ray particles calculation with tabulated results for 79 points on earth surface
Fowler, B. C.↗
Variability of Centaurus XR-2.
X ray flux variability from Centaurus XR-2 object detected by Skylark rocketborne proportional counters
Fenton, A. G.↗
Cosmic-ray propagation processes. I.
Time dependency, anisotropy, propagation and spectral properties of cosmic radiation released by solar flares during sunspot activity
SUNSPOT CYCLE↗
Cosmic-ray propagation processes. II.
Intense fluxes of charged particles associated with disturbances in interplanetary medium during 1966
SOLAR FLARE↗
Cosmic-ray propagation processes. III.
Cosmic ray propagation processes studied from measurement of anisotropic character of cosmic radiation /1965-1966/
DIURNAL VARIATION↗
A strong X-ray source in the vicinity of the constellation Crux.
Strong X-ray source in vicinity of constellation Crux compared to SCO xr-1, findings suggest similar physical nature
SCORPIO CONSTELLATION↗
Pioneer VI observations of the solar flare particle event of 7 July, 1966.
Time dependency, anisotropy degree and spectral composition of cosmic radiation generated during July 1966 solar flares as observed by Pioneer VI
SOLAR FLARE↗
Upper limits to the hard X-ray flux from the quiet sun and Jupiter.
Upper limits to hard X-ray flux from quiet sun analyzed by balloon-borne scintillation detector measuring celestial sources
BALLOON SOUNDING↗
A digital system for accurate time sector division of a spin-stabilized vehicle.
Aspect system on Pioneer VI and VII INCORPORATES digital computer for accurate time sector division of spin stabilized vehicle
SPIN STABILIZATION↗
The cosmic radiation anisotropy as a separable function of time and radiation.
Cosmic radiation anisotropy variation with time and direction described on intensity contour map, noting application for neutron monitors data reduction
ANISOTROPY↗
Pioneer VI detector to measure degree of anisotropy of cosmic radiation in energy range 7.5-90 MEV/nucleon.
Pioneer VI detector to measure degree of anisotropy of cosmic radiation at various energy ranges
ENERGY LEVEL↗
Energy spectra of a number of celestial X-ray sources in the energy range from 2 to 60 kiloelectron volts.
Energy spectrum of X-ray source in Cygnus constellation with 2 to 60 kev
ENERGY SPECTRUM↗
Recurrent Forbush decreases associated with M-region magnetic storms.
Recurrent cosmic-ray modulation phenomena with Forbush decrease characteristics correlated with M-region magnetic storms, concluding that each series results from shock wave solar initiated
COSMIC RADIATION↗
Anisotropic cosmic radiation fluxes of solar origin.
Anisotropic cosmic radiation with flare effects flowing out of Sun and along filamentary magnetic structures imbedded in solar wind
SOLAR WIND↗