The isotopic composition of solar flare accelerated neon

Details The isotopic composition of solar flare accelerated neon The isotopic composition of solar flare accelerated neon

Jul 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...231l..97m&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 231, July 15, 1979, p. L97-L100.

Astronomy and Astrophysics

Astrophysics

25

Abundance, Heavy Nuclei, Neon Isotopes, Particle Acceleration, Solar Cosmic Rays, Solar Flares, Meteoritic Composition, Particle Telescopes, Solar Wind

Scientific paper

The individual isotopes of neon in energetic solar-flare particles have been clearly resolved with a rms mass resolution of 0.20 amu. The ratios found are Ne-20/Ne-22 = 7.6 (+2.0, -1.8) and Ne-21/Ne-22 of no more than about 0.11 in the 11-26 MeV per nucleon interval. This isotopic composition is essentially the same as that of meteoritic planetary neon-A and is significantly different from that of the solar wind.

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