The MG II H line in sunspot umbrae

Details The MG II H line in sunspot umbrae The MG II H line in sunspot umbrae

Jan 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984soph...90...13g&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 90, Jan. 1984, p. 13-15.

Physics

7

H Lines, Solar Spectra, Sunspots, Ultraviolet Spectra, Umbras, Chromosphere, Solar Maximum Mission, Spectral Energy Distribution

Scientific paper

Solar Maximum Mission UVSP observations of the Mg II h line in the
umbrae of five sunspots show a spread of a factor of 3 in peak
intensity. It is concluded that this range is larger than and brackets
the range found in a single umbra by Lites and Skumanich (1982).

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