A search for alpha particles trapped in the geomagnetic field.
Alpha particle proton ratio of geomagnetic field from data from charged-particle telescope on OGO 1 satellite
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Alpha particle proton ratio of geomagnetic field from data from charged-particle telescope on OGO 1 satellite
Observation of short period pulsations of earth geomagnetic field with fluxmetric induction - earth current measurements
Computations concerning variations of the geomagnetic field at MAGSAT altitudes were investigated. Using MAGSAT data for the X, Y, and Z components of the geomagnetic field, a computer conversion to yield the H component was performed. Two methods of determining delta H normalized to a constant geocentric distance R sub 0 = 6800 were investigated, and the utility of elta H at times of magnetic storms was considered. Delta H at a geographical latitude of 0 at dawn and dusk, the standard Dst, and K sub p histograms were plotted and compared. Magnetic anomalies are considered. Examination of data from the majority of the 400 passes of MAGSAT considered show a reasonable delta H versus latitude variation. Discrepancies in values are discussed.
Computation of main geomagnetic field from spherical harmonic expansions
Computing cosmic ray cutoff rigidity for several geomagnetic field models
Quiet condition solar wind geomagnetic field interaction measurements, discussing solar plasma and bow shock wave generation
By modifying the IGRF it is possible to learn what may happen to the geomagnetic field during a geomagnetic reversal. If the entire IGRF reverses then the declination and inclination only reverse when the field strength is zero. If only the dipole component of the IGRF reverses a large geomagnetic field remains when the dipole component is zero and he direction of the field at the end of the reversal is not exactly reversed from the directions at the beginning of the reversal.
Main geomagnetic field role in conjugate points location
Ionospheric focusing for antenna in geomagnetic field, using geometrical optics
Nondipole part of geomagnetic field located at magnetosphere boundary
Computation of geomagnetic cosmic-ray cutoff rigidities
The importance of global geomagnetic field models for the reduction of magnetic surveys is discussed. It is demonstrated that a numerical model with adequate secular variation correction, provides a suitable representation of the regional field. The limitations of the presently available models are reported, with emphasis on the International Geomagnetic Reference Field.
Explorer VI satellite observations of geomagnetic field fluctuations and perturbations
Mapping the magnetosphere on a dipole geomagnetic field model by projecting field and particle observations onto the model is described. High-latitude field lines are traced between the earth's surface and their intersection with either the equatorial plane or a cross section of the geomagnetic tail, and data from low-altitude orbiting satellites are projected along field lines to the outer magnetosphere. This procedure is analyzed, and the resultant mappings are illustrated. Extension of field lines into the geomagnetic tail and low-altitude determination of the polar cap and cusp are presented. It is noted that while there is good agreement among the various data, more particle measurements are necessary to clear up statistical uncertainties and to facilitate comparison of statistical models.
Low frequency hydromagnetic waves in distant geomagnetic field - explorer vi satellite
Distant geomagnetic field - hydromagnetic disorder and shocks in magnetopause
Fluid mechanics model representation of solar wind and geomagnetic field interaction, noting flow parameters in shock layer and application of MHD EQUATIONS
Low-frequency hydromagnetic waves in geomagnetic field - data obtained from magnetometer, aspect indicator and scintillation counter on explorer 6 satellite