Published April 25, 1975 | Version v1
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Unusual emission of iron nuclei from the Sun

Creators

Description

Sustained emission of low energy solar particles with a composition richer in iron than oxygen is observed in the time period 1974 May 7 to 17. Between 0.7 and 4 MeV/nucleon the relative abundances of C:O:Fe are 0.24:1:1.35. It was suggested that these observations provide indication for effects of heavy ion enrichment in the lower corona of the sun. (auth)

Availability note (English)

MF available from INIS under the Report Number.

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Additional details

Publishing Information

Imprint Pagination
14 p.
Report number
N--75-23450

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
7231927
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
ATOMIC NUMBER; CARBON; CHEMICAL COMPOSITION; ENERGETIC SOLAR PARTICLES; IRON; OXYGEN; SOLAR CORONA
Descriptors DEC
ELEMENTS; METALS; NONMETALS; RADIATIONS; SOLAR RADIATION; STELLAR RADIATION; TRANSITION ELEMENTS

Optional Information

Secondary number(s)
NASA-CR--142712.