Stationary microvariation station with photoelectronic amplification
Geomagnetic field microvariation measurement using photoelectronic amplification
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Geomagnetic field microvariation measurement using photoelectronic amplification
Indices of solar & geomagnetic activity, variation of earth magnetic field in time & space, & field variation in magnetic storm
Analysis of explorer vi & pioneer v data on radiation belts & geomagnetic field
Motion of low rigidity cosmic rays in dipole field - geomagnetic and external fields
Pulsating auroras as source of infrasonic waves associated with geomagnetic activity
Sporadic ionospheric e-layer effect on daily variations of geomagnetic field
Spatial model of geomagnetic field of effective solar corpuscular flux based on mariner ii measurements
Geomagnetic polar region - arrival of extraterrestrial low energy protons
The idealized model of the geomagnetic field-solar wind interaction yields a singular (neutral) point on the magnetopause at which the magnetic field vanishes. If we expand the fields in a power series around this point, including quadratic terms, we can derive an approximate equation of the magnetopause in a small neighborhood of the neutral point which is consistent with the idealized boundary conditions to fourth order. We then consider the additional pressure due to multiple reflections of particles in this neighborhood and show that less than a 4 per cent correction to the single-reflection pressure condition is necessary.
Ring current effects on axisymmetric development of geomagnetic storm fields in low and middle latitudes
Upper atmosphere heating in auroral zones during geomagnetic perturbations - analysis of atmospheric drag data from injun iii satellite
Role of flare-like nonstationary processes in origin of solar wind from analysis of geomagnetic disturbances
Duration of geomagnetic variations as function of latitude - k index variations
Cosmic ray cutoff in the stormer sense for high latitudes at which the geomagnetic field is approximately axisymmetric
Effect of solar activity, diurnal, semiannual and annual density variation, and geomagnetic activity on upper atmosphere, analyzed from orbital period fluctuations of artificial satellites
Solar neutron decay indicates important source of geomagnetically trapped particles of inner and outer radiation belts
Ring current effects on asymmetric development of geomagnetic storm fields in low and middle latitudes
Explorer ix satellite drag data analysis, observing atmospheric temperature perturbations due to geomagnetic storms