Add to ORKGProtons associated with centers of solar activity and propagation in interplanetary magnetic field regions co-rotating with su
Data from the Far Ultraviolet Imager (FUV) on the Imager for Magnetopause-to-Aurora Global Explorati...
Magnetic field gradient and rotating motions of sunspot groups and effects on solar proton flare
The Earth receives all of its external energy input from the Sun (except for galactic sources), whic...
The relation of the coronal magnetic field structure to the distribution of approximately 1 MeV prot...
Recurrent low energy ( ≳0.5 MeV) proton flux enhancements, reliable indicators of corotating plasma ...
From December 1975 to June 1976 we observed an evolving recurrent proton enhancement with IMP 7/8 ...
International audienceSolar energetic particle fluxes (Ee > 38 keV) observed by the ULYSSES/HI-SCALE...
The access of 1.2 to 40 MeV protons and 0.4 to 1.0 MeV electrons from interplanetary space to the po...
The existence of interplanetary flow systems produced by the entrainment of interplanetary transient...
Pioneer 6 observations of proton flare ejected magnetic bottles are reported. The SSC geomagnetic st...
International audienceIn this work, solar flare energetic particle fluxes (Ee ? 42 keV) observed by ...
A statistical study of the initial phases of 185 solar particle events was carried out using the dat...
Solar and solar induced phenomena during twentieth solar cycle measured by satellites and space prob...
From the data on solar protons with energy 0.3 MeV obtained by Explorer 35 since July 1967, ten eve...
Seven solar flares that were followed by major proton events were examined to determine the diverse ...
Data from the Far Ultraviolet Imager (FUV) on the Imager for Magnetopause-to-Aurora Global Explorati...
Magnetic field gradient and rotating motions of sunspot groups and effects on solar proton flare
The Earth receives all of its external energy input from the Sun (except for galactic sources), whic...
The relation of the coronal magnetic field structure to the distribution of approximately 1 MeV prot...
Recurrent low energy ( ≳0.5 MeV) proton flux enhancements, reliable indicators of corotating plasma ...
From December 1975 to June 1976 we observed an evolving recurrent proton enhancement with IMP 7/8 ...
International audienceSolar energetic particle fluxes (Ee > 38 keV) observed by the ULYSSES/HI-SCALE...
The access of 1.2 to 40 MeV protons and 0.4 to 1.0 MeV electrons from interplanetary space to the po...
The existence of interplanetary flow systems produced by the entrainment of interplanetary transient...
Pioneer 6 observations of proton flare ejected magnetic bottles are reported. The SSC geomagnetic st...
International audienceIn this work, solar flare energetic particle fluxes (Ee ? 42 keV) observed by ...
A statistical study of the initial phases of 185 solar particle events was carried out using the dat...
Solar and solar induced phenomena during twentieth solar cycle measured by satellites and space prob...
From the data on solar protons with energy 0.3 MeV obtained by Explorer 35 since July 1967, ten eve...
Seven solar flares that were followed by major proton events were examined to determine the diverse ...
Data from the Far Ultraviolet Imager (FUV) on the Imager for Magnetopause-to-Aurora Global Explorati...
Magnetic field gradient and rotating motions of sunspot groups and effects on solar proton flare
The Earth receives all of its external energy input from the Sun (except for galactic sources), whic...