Add to ORKGSolar proton fluxes have been deduced from Al-26 depth profile resulting mainly from their interactions with Mg, Al and Si in lunar rocks. After correcting for lunar orientation, erosion and exposure age, as determined from the track density profile, the Al-26 profile is found to yield a flux which can be represented by (Js ,Ro )=(125,125). This value is also consistent with the Al-26 depth profile in lunar soil columns. The data also indicate that the solar proton flux has remained nearly constant during last few million years
Ph.D. University of Hawaii at Manoa 2014.Includes bibliographical references.This dissertation is fo...
The long term variations of the intensity of solar cosmic rays, galactic cosmic rays, and the solar ...
Abstract Direct measurements of solar energetic particles (SEP) became possible only in the space e...
Solar proton fluxes have been deduced from Al-26 depth profile resulting mainly from their interacti...
The solar flare proton fluxes, averaged over different periods of time, have been determined from Al...
We determined concentration profiles of Ne-21, Ne-22, and Ar-38 produced by solar protons as a funct...
A nondestructive beta-gamma coincidence technique was used to measure the radioactivity of lunar roc...
Abstract Aims: Lunar soil and rocks are not protected by a magnetic field or an atmosphere and are c...
Abstract Direct measurements of solar energetic particles (SEP) cover the space era of several deca...
Aims. Lunar soil and rocks are not protected by a magnetic field or an atmosphere and are continuous...
Abstract. A statistical analysis of the contemporary (1954–1975) solar flare particle events has bee...
The authors have measured the concentrations of Al-26 in lunar rock samples 15555,859 and 60025,28 w...
Cosmic rays penetrate the lunar surface and interact with the lunar rocks to produce both radionucli...
Recent results on cosmic ray interactions in lunar samples and meteorites resulting in productio...
The authors have measured the concentrations of 26Al in lunar rock samples 15555,859 and 60025,28 wi...
Ph.D. University of Hawaii at Manoa 2014.Includes bibliographical references.This dissertation is fo...
The long term variations of the intensity of solar cosmic rays, galactic cosmic rays, and the solar ...
Abstract Direct measurements of solar energetic particles (SEP) became possible only in the space e...
Solar proton fluxes have been deduced from Al-26 depth profile resulting mainly from their interacti...
The solar flare proton fluxes, averaged over different periods of time, have been determined from Al...
We determined concentration profiles of Ne-21, Ne-22, and Ar-38 produced by solar protons as a funct...
A nondestructive beta-gamma coincidence technique was used to measure the radioactivity of lunar roc...
Abstract Aims: Lunar soil and rocks are not protected by a magnetic field or an atmosphere and are c...
Abstract Direct measurements of solar energetic particles (SEP) cover the space era of several deca...
Aims. Lunar soil and rocks are not protected by a magnetic field or an atmosphere and are continuous...
Abstract. A statistical analysis of the contemporary (1954–1975) solar flare particle events has bee...
The authors have measured the concentrations of Al-26 in lunar rock samples 15555,859 and 60025,28 w...
Cosmic rays penetrate the lunar surface and interact with the lunar rocks to produce both radionucli...
Recent results on cosmic ray interactions in lunar samples and meteorites resulting in productio...
The authors have measured the concentrations of 26Al in lunar rock samples 15555,859 and 60025,28 wi...
Ph.D. University of Hawaii at Manoa 2014.Includes bibliographical references.This dissertation is fo...
The long term variations of the intensity of solar cosmic rays, galactic cosmic rays, and the solar ...
Abstract Direct measurements of solar energetic particles (SEP) became possible only in the space e...