Energetic particles from the Sun have only been studied in detail during the last three decades. The modern record is good, although the number of the largest solar particle events are very few. The nuclides made by solar energetic particles in lunar rocks have been used to extend the record of these particles {approximately} 10{sup 7} years. The modern and ancient records are similar. By combining both sets of data, it has been inferred that solar particle events much larger than the largest events observed during the last four solar cycles are very rare
The very large solar proton events, those having an omni-directional solar proton fluence greater th...
The very large solar proton events, those having an omni-directional solar proton fluence greater th...
AbstractIn this study, all available data on the largest solar proton events (SPEs), or extreme sola...
Modern solar energetic particles (SEPs) have been studied for about 50 years by satellites and groun...
Several sets of measurements of the fluxes of solar energetic particles (SEPs) above 10 MeV have bee...
Abstract The era of direct or indirect (ground-based) observations of solar energetic particle (SEP...
The probability of occurrence of extreme solar particle events (SPEs) with proton fluence (>30 Me...
Aims. Lunar soil and rocks are not protected by a magnetic field or an atmosphere and are continuous...
Aims. Lunar soil and rocks are not protected by a magnetic field or an atmosphere and are continuous...
Aims. Lunar soil and rocks are not protected by a magnetic field or an atmosphere and are continuous...
It has long been known that the great majority of nuclear active solar particles are emitted in a fe...
Abstract Aims: Lunar soil and rocks are not protected by a magnetic field or an atmosphere and are c...
[1] A possible contribution of solar energetic particle events to the production of cosmogenic 10Be ...
The very large solar proton events, those having an omni-directional solar proton fluence greater th...
Abstract The Sun sporadically produces eruptive events leading to intense fluxes of solar energetic...
The very large solar proton events, those having an omni-directional solar proton fluence greater th...
The very large solar proton events, those having an omni-directional solar proton fluence greater th...
AbstractIn this study, all available data on the largest solar proton events (SPEs), or extreme sola...
Modern solar energetic particles (SEPs) have been studied for about 50 years by satellites and groun...
Several sets of measurements of the fluxes of solar energetic particles (SEPs) above 10 MeV have bee...
Abstract The era of direct or indirect (ground-based) observations of solar energetic particle (SEP...
The probability of occurrence of extreme solar particle events (SPEs) with proton fluence (>30 Me...
Aims. Lunar soil and rocks are not protected by a magnetic field or an atmosphere and are continuous...
Aims. Lunar soil and rocks are not protected by a magnetic field or an atmosphere and are continuous...
Aims. Lunar soil and rocks are not protected by a magnetic field or an atmosphere and are continuous...
It has long been known that the great majority of nuclear active solar particles are emitted in a fe...
Abstract Aims: Lunar soil and rocks are not protected by a magnetic field or an atmosphere and are c...
[1] A possible contribution of solar energetic particle events to the production of cosmogenic 10Be ...
The very large solar proton events, those having an omni-directional solar proton fluence greater th...
Abstract The Sun sporadically produces eruptive events leading to intense fluxes of solar energetic...
The very large solar proton events, those having an omni-directional solar proton fluence greater th...
The very large solar proton events, those having an omni-directional solar proton fluence greater th...
AbstractIn this study, all available data on the largest solar proton events (SPEs), or extreme sola...