On the effect of resonant magnetic-moment violation on trapped particles
Effect of resonant magnetic moment violation on geomagnetically trapped particles
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Effect of resonant magnetic moment violation on geomagnetically trapped particles
Trapped charged particle motion in geomagnetic field distorted by solar wind
Betatron acceleration effects on intensity and energy spectrum of magnetically trapped particles
Determination of diaphragm opening-times and use of diaphragm particle traps in hypersonic shock tube
Magnetospheric electric field configuration from trapped particle flux asymmetries, using Explorer 14 electron data
Computer program to calculate geomagnetically trapped particle shell model, drift rate, and bounce paths
Tabulation of spherical harmonic coefficients of geomagnetic field data for trapped-particle evaluation
Radial diffusion of trapped particles due to large spatial scale magnetic disturbances, considering arbitrary pitch angle
Long term variations in high energy geomagnetically trapped particles from satellite detector data
Some field-geometric features of relevance to particle trapping in the inner magnetosphere and polar-cap regions of Jupiter are described using an internal-field model that includes terms up to the order of n equals 3 (octupole). Adiabatic particle parameters for detectors on Pioneers 10 and 11 during their flights through Jupiter's inner magnetosphere are determined along with the configuration of the intersections of particle drift shells with the planetary ionosphere. Possible correlations between drift-shell contours and the planet-locked characteristics of Jovian decametric radio emission are investigated, and longitudinal asymmetries of the ionospheric plasma source function are analyzed. It is shown that if the ionosphere is the main source of magnetospheric plasma, the latitude dependence of the plasma source function should have a considerable effect on the longitudinal asymmetry of the corotating plasma.
Data from explorer xiv satellite concerning the absolute intensities of geomagnetically trapped particles and the outer boundary of the magnetosphere
The NAIRAS(Nowcast of Aerospace Ionizing RAdiation system) model was initially developed for fast computation of GCR and SEP events in the Earth's atmosphere. It was recently improved for computing the effects of trapped particles and its domain of validity was extended to the near space environments, which notably includes the international space station (ISS). To validate the new capabilities of the model, we compared its outputs with some measurements made in the ISS. Historical data contained several SEP events while newer measurements made with the ARMAS instrument flying in the experience bay of KIBO show the influence of trapped particles and GCR over the total dose received.
Polar substorm particle event observed with magnetic field and trapped particle detectors on Explorer 26 during April 1965 worldwide magnetic storm
Particle trapping and plasma oscillations in satellite disturbed ionosphere observed from Ariel and Alouette measurements, discussing frequency and wavelength relation
Alpha particle proton ratio of geomagnetic field from data from charged-particle telescope on OGO 1 satellite
Satellite observation of alpha particles trapped geomagnetically in radiation belts, including Injun 5 results
Acceleration of trapped particles during magnetic storm on 18 Apr. 1965 observed by Explorer 26
Observations of interplanetary magnetic field fluctuations in correlation with trapped particle fluctuations are discussed. From observations of particle-redistribution effects, properties of the magnetospheric electric field are derived. The obtained results suggest that the interplanetary B(sub z) field fluctuations might represent a strong driving source for particle diffusion.