Magnetosheath field, geomagnetic index a sub p and stability of magnetopause.
Magnetosheath field, geomagnetic activity index, magnetopause stability and interplanetary magnetic field influence on magnetospheric phenomena
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Magnetosheath field, geomagnetic activity index, magnetopause stability and interplanetary magnetic field influence on magnetospheric phenomena
Explorer 34 plasma experiment data on solar wind-magnetosheath boundary
Electron pulses and magnetic fields in magnetosheath and beyond bow shock studied for correlation by IMP 1 satellite
Pioneer 6 observations of steady state magnetosheath during transit of magnetopause under quiet solar wind-geomagnetic field interaction conditions
Magnetosheath-solar wind boundary discontinuous transitions in proton spectrum, flow direction and magnetic flux from Explorer 34 satellite data
Spatial characteristics of magnetic field in earth magnetosheath
Noise signals in earth magnetosheath interpreted as electromagnetic waves propagating in whistler mode
Pioneer 6 plasma measurements in magnetosheath
Pioneers 7 and 8 space probes of magnetic fields fluctuations in magnetosheath
Magnetic field fluctuations in magnetosheath of Explorer 34 spectral data on sunward earth hemisphere
Spatial characteristics of magnetosheath magnetic field observed simultaneously by Explorer satellites, showing zero order agreement with prediction of MGD theory
Earth magnetosphere and magnetosheath magnetic field measurements by Mariner 5
Magnetosheath plasma measurements by Pioneer 6 during outbound passage in dusk meridian, comparing results with various predictions
Magnetic and electric field changes across earth bow shock and magnetosheath, discussing Pioneer 8 and OGO-5 data
Steady state magnetic and electric fields in magnetosheath by linear superposition of field vectors, using axisymmetric velocity function from gas dynamics
Magnetic field fluctuations in magnetosheath from Pionner observations, noting bow shock correlation
Sunward magnetosheath magnetic field fluctuations, noting power levels spatial variations, transverse shock aligned fields and longitudinal waves
Magnetosheath plasma penetrating to low altitudes in the dayside cusp region of the magnetosphere has been observed by the ISIS 1 soft particle spectrometer (SPS). The extent of these particle fluxes in local magnetic time and invariant latitude, their variation with magnetic activity, and their pitch angle distribution are given. Comparison between the SPS data and energetic particle data indicates that the boundary between open and closed field lines on the dayside is associated with a sharp drop in the outer zone keV electron fluxes. It is shown that these newly identified cusp fluxes provide the necessary energy to produce observed dayside auroral oval phenomena.