Active solar radio regions at metric frequencies and the interplanetary sector structures
Metric frequency solar radio noise active regions relationship to interplanetary magnetic field polarity distribution
Engineering topics
Publications and source records attributed to Sakurai, K..
Metric frequency solar radio noise active regions relationship to interplanetary magnetic field polarity distribution
Active region MacMath no. 8905 proding 16 distinct electron events associated with solar flares during passage across solar disk
Magnetic field gradient and rotating motions of sunspot groups and effects on solar proton flares
Relativistic electrons associated with solar flares and type 1 noise storms
Solar cosmic ray acceleration and propagation from time variation and heliocentric distance dependence of relative abundance of protons to helium nuclei
Relativistic electrons acceleration in solar proton flares, taking into account plasma density and magnetic field intensity
Type 3 radio bursts at hectometric wavelengths from 13 to 25 August 1968, noting effect of large active sunspot groups
Energetic electrons generating solar flares position relation with active regions associated with type I radio noise storms
Active solar radio regions at metric frequencies and interplanetary sector structures
Stability of sunspot magnetic fields and origin of solar flares
Acceleration and propagation of solar cosmic rays as deduced from relative abundance of protons to helium nuclei
Gyrosynchrotron radiation transfer in magnetoactive plasma
Acceleration of relativistic electrons in solar proton flares
Energetic electrons associated with solar flares and their relation to type 1 noise activity
Characteristics of solar active regions responsible for generation of type 3 radio bursts at hectometric frequencies in Aug. 1968
Rotating motion of sunspot groups associated with solar proton flare
X ray and H alpha emissions associated with solar proton flares, correlating rise time with solar cosmic rays
H alpha brightening areas related to sunspot magnetic fields configuration and solar proton flares