Spectroscopic detection of solar He-3

Details Spectroscopic detection of solar He-3 Spectroscopic detection of solar He-3

Apr 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...197..509h&link_type=abstract

Astrophysical Journal, vol. 197, Apr. 15, 1975, pt. 1, p. 509-512.

Astronomy and Astrophysics

Astrophysics

21

Helium Isotopes, Infrared Spectra, Solar Prominences, Solar Spectra, Abundance, Astronomical Spectroscopy, Deuterium, Light Elements, Line Spectra, Luminous Intensity, Photosphere, Solar Limb, Stellar Evolution

Scientific paper

Excess emission in the longward wing of the 10830-A helium feature in a
solar prominence is identified as due to solar He-3. A solar
(He-3)/(He-4) abundance ratio of .0004 plus or minus .0002 is obtained,
and its implications are discussed.

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