Add to ORKGProton detection of approximately 500 KeV kinetic energy by Mariner IV Space Probe during interplane...
The vertical geomagnetic cutoffs for cosmic-ray protons are presented for seven different energy int...
The variations in the equatorial penetration boundary of solar protons with E sub p = 0.9 to 8.0 MeV...
In the Earth's polar regions the intensity of the solar protons with the energy above the critical e...
The access of 1.2 to 40 MeV protons and 0.4 to 1.0 MeV electrons from interplanetary space to the po...
[[abstract]]Solar proton events have been recorded based on the criteria when the proton fluxes at e...
Proton and electron intensity maps from outer radiation zone measurements by electrostatic analyzer ...
Explorer xii ion-electron detection in magnetic storm sudden commencement on sept 30 1961 - 0.1 to 5...
A proton of low energy moving in the equatorial plane of the earth will experience drift motions due...
Temporal variations of 40 keV electrons in magnetosphere during and after magnetic storm on April 18...
Explorer XXVIII and XXXIII and Pioneer VI MAGNETOMETRIC determination of general macrostructure of ...
Ratio of intensity of solar protons for north polar cap to that of south polar cap, as observed by E...
The Earth receives all of its external energy input from the Sun (except for galactic sources), whic...
Temporal variations of 100 keV to 1700 keV trapped protons from data recorded by scintillation count...
The access of 1.2-40 MeV protons and 0.4-1.0 MeV electrons from interplanetary space to the polar c...
Proton detection of approximately 500 KeV kinetic energy by Mariner IV Space Probe during interplane...
The vertical geomagnetic cutoffs for cosmic-ray protons are presented for seven different energy int...
The variations in the equatorial penetration boundary of solar protons with E sub p = 0.9 to 8.0 MeV...
In the Earth's polar regions the intensity of the solar protons with the energy above the critical e...
The access of 1.2 to 40 MeV protons and 0.4 to 1.0 MeV electrons from interplanetary space to the po...
[[abstract]]Solar proton events have been recorded based on the criteria when the proton fluxes at e...
Proton and electron intensity maps from outer radiation zone measurements by electrostatic analyzer ...
Explorer xii ion-electron detection in magnetic storm sudden commencement on sept 30 1961 - 0.1 to 5...
A proton of low energy moving in the equatorial plane of the earth will experience drift motions due...
Temporal variations of 40 keV electrons in magnetosphere during and after magnetic storm on April 18...
Explorer XXVIII and XXXIII and Pioneer VI MAGNETOMETRIC determination of general macrostructure of ...
Ratio of intensity of solar protons for north polar cap to that of south polar cap, as observed by E...
The Earth receives all of its external energy input from the Sun (except for galactic sources), whic...
Temporal variations of 100 keV to 1700 keV trapped protons from data recorded by scintillation count...
The access of 1.2-40 MeV protons and 0.4-1.0 MeV electrons from interplanetary space to the polar c...
Proton detection of approximately 500 KeV kinetic energy by Mariner IV Space Probe during interplane...
The vertical geomagnetic cutoffs for cosmic-ray protons are presented for seven different energy int...
The variations in the equatorial penetration boundary of solar protons with E sub p = 0.9 to 8.0 MeV...