Polar solar daily geomagnetic variations on exceptionally quiet days.
Polar solar diurnal geomagnetic variations on quiet days noting polar field distribution
Akasofu, S.-I.↗
Engineering topics
Akasofu, S.-I.
Publications and source records attributed to Akasofu, S.-I..
The geomagnetic storm of April 17-18, 1965.
Growth and decay of geomagnetic storms of April 17-18, 1965 studied using data from 88 ground stations, Explorer XXVI and Vela satellites
GEOMAGNETIC STORM↗
Polar magnetic substorm in the evening sector.
Evening sector polar magnetic substorm disturbance field morphology in transition region
POLAR CAP↗
Intense negative bays inside the auroral zone. I.
Intense negative bays occurring in auroral zone in early evening hours explained by westward extension of polar electrojet
AURORAL ZONE↗
Auroral activity in the evening sector.
Evening auroral activity characterized by westward traveling surges occurring not within auroral zone center
GEOPHYSICS↗
The abnormally early appearance of the eastward motion of auroras in the evening.
Abnormally early eastward auroral motion appearance in evening and associated magnetospheric plasma shell motion
AURORAL ZONE↗
A systematic shift of the DS axis.
Systematic clockwise rotation of asymmetry axis of main phase decrease during geomagnetic storm lifetime
GEOMAGNETIC STORM↗
On the three dimensional structure of the solar plasma flow generated by solar flares.
Three-dimensional structure of solar plasma flow generated by solar flares, noting geometric factors in geomagnetic storm intensity decrease
PLASMA FLOW↗
The structure of the solar plasma flow generated by solar flares.
Geomagnetic storms due to solar flares statistically analyzed to obtain configuration of solar plasma flow generated by solar flares
GEOMAGNETIC STORM↗
The normality of the SD variation at Huancayo and the asymmetry of the main phase of geomagnetic storms.
Normality of SD variation at dip-equatorial stations suggests origin beyond F layer
F LAYER↗
The auroral oval and the internal structure of the magnetosphere.
Auroral oval between outer boundary of trapping region and ionosphere and dynamical and atomic interactions between magnetospheric plasma and neutral atmosphere
E LAYER↗
The significance of the multiple structure of the auroral arc.
Interpretation of multiple structure of auroral arc
CURRENT SHEET↗
Electrodynamics of the magnetosphere - Geomagnetic storms.
Geomagnetic and auroral storms provide information on interaction of solar plasma flows and magnetosphere
MAGNETOSPHERE↗
Dynamics of the aurora. VII - Equatorward motions and the multiplicity of auroral arcs.
Equatorward motions of auroras
AURORA↗
The auroral oval, the auroral substorm, and their relations with the internal structure of the magnetosphere.
Auroral oval, auroral substorm and relations with internal magnetospheric structure during growth and decay of ring current and neutral sheet current
AURORAL ACTIVITY↗
Electrodynamics of the magnetosphere - Geomagnetic storms
Electrodynamics of interaction between solar plasma flow and magnetosphere producing geomagnetic storms
SOLAR PLASMA↗
Dynamics of the aurora. IV - Polar magnetic substorms and westward traveling surges.
Polar magnetic substorms associated with westward traveling surge
POLAR AURORA↗