On the motion of charged particles in the geomagnetic field

1963 ◽  
Vol 24 ◽  
pp. 1-18 ◽  
Author(s):  
Ernest C Ray
1985 ◽  
Vol 63 (4) ◽  
pp. 445-452
Author(s):  
R. N. Singh ◽  
R. Prasad

In addition to parallel electric fields, the distortions in the geomagnetic field have been considered in the study of resonant whistler wave interaction with gyrating charged particles. Mead axisymmetric distortions in the geomagnetic field have been considered and new expressions for the inhomogeneity parameter, αd, have been obtained. Considering the diffusion of charged particles in pitch angle, the variation in the precipitating electron flux under varying magnetospheric conditions has been computed. The variation in the distribution of trapped charged particles is shown to play an important role in controlling the electron flux precipitated into the lower ionosphere.


Although superficially very much like its predecessor Ariel 3, a partial change in the experiment payload produced in Ariel 4 a cheap and ‘mission oriented’ satellite - that is to say, one in which all experiments contribute to the same investigation. The group objective of the Ariel 4 experiments was to examine the relation between naturally occurring radio frequency noise in the ionosphere and the influx of high energy charged particles, measured at the same time and place. The data handling system was designed to facilitate this objective. Each experiment could however make a separate contribution to other aspects of space research. Special technical compatibility problems were overcome and attitude control was achieved using the reaction between a current carrying coil and the geomagnetic field.


2021 ◽  
pp. 27-61
Author(s):  
Hannu E. J. Koskinen ◽  
Emilia K. J. Kilpua

AbstractIn this chapter we discuss the concepts that govern the motion of charged particles in the geomagnetic field and the principles how they stay trapped in the radiation belts. The basic particle orbit theory can be found in most plasma physics textbooks. We partly follow the presentation in Koskinen (Physics of space storms, from solar surface to the earth. Springer-Praxis, Heidelberg, 2011). A more detailed discussion can be found in Roederer and Zhang (Dynamics of magnetically trapped particles. Springer, Heidelberg, 2014). A classic treatment of adiabatic motion of charged particles is Northrop (The adiabatic motion of charged particles. Interscience Publishers, Wiley, New York, 1963).


Atmosphere ◽  
2021 ◽  
Vol 12 (12) ◽  
pp. 1600
Author(s):  
Michael Hanzelka ◽  
Jiří Dan ◽  
Pavel Fiala ◽  
Přemysl Dohnal

We evaluate the impact of changes in solar activity on three significant human psychophysiological parameters: skin conductance, electromyography (EMG), and the share of abdominal and diaphragmatic breathing in overall ventilation. Variations affecting human psychophysiology due to changes in solar activity directly document the assertion that psychology, behavior, and decision-making all reflect geomagnetic field alterations that stem from variable solar activity. The relevant experiments showed that solar processes, during which the Earth is exposed to electrically charged particles from the Sun (solar wind), exert an impact on the psychophysiological parameters of the body.


1984 ◽  
Vol 75 ◽  
pp. 203-209
Author(s):  
Joseph A. Burns

ABSTRACTLying in Jupiter's equatorial plane is a diaphanous ring having little substructure within its three components (main band, faint disk, and halo). Micron-sized grains account for much of the visible ring, but particles of centimeter sizes and larger must also be present to absorb charged particles. Since dynamical evolution times and survival life times are quite short (≲102-3yr) for small grains, the Jovian ring is being continually replenished; probably most of the visible ring is generated by micrometeoroids colliding into unseen parent bodies that reside in the main band.


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