On a cold emission in the solar corona

Details On a cold emission in the solar corona On a cold emission in the solar corona

Mar 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975soph...41...89a&link_type=abstract

Solar Physics, vol. 41, Mar. 1975, p. 89-95.

Physics

1

Emission Spectra, Line Spectra, Solar Corona, Solar Prominences, Solar Temperature, Coronagraphs, Electron Density (Concentration), H Lines, Helium, K Lines, Solar Spectra

Scientific paper

The faint emission of hydrogen, helium and metals in the corona which
appeared near an active prominence is studied. The calculations showed
that the temperature of the emission region is in the limits from 10,000
K to 30,000 K and the electron density is between 1 billion and 10
billion per cu cm, respectively.

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