The abundances of ultraheavy nuclei in solar energetic particles

Details The abundances of ultraheavy nuclei in solar energetic particles The abundances of ultraheavy nuclei in solar energetic particles

Mar 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990aipc..203..255w&link_type=abstract

IN: Particle astrophysics - The NASA cosmic ray program for the 1990s and beyond (A92-20526 06-93). New York, American Institute

Astronomy and Astrophysics

Astrophysics

Abundance, Heavy Nuclei, Solar Corpuscular Radiation, Solar Flares, Energetic Particles, Particle Acceleration, Particle Energy, Radiation Detectors

Scientific paper

It is noted that measurement of the elemental and isotopic composition of nuclei accelerated in solar flares is important both as a probe of physical conditions at the acceleration location and as a source of data on the composition of solar surface material and of the presolar nebula from which it was acquired. To obtain information on the rare 'ultraheavy' (Z more than 28) elements, it is necessary to develop large area detectors. Suitable sites for conducting these types of measurements include a dedicated satellite outside the earth's magnetosphere, a lunar base, and a polar platform in LEO.

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