The large-scale behaviour of the green emission corona FeXIV 530.3 NM over the last 4.5 solar activity cycles

Details The large-scale behaviour of the green emission corona FeXIV 530.3 NM over the last 4.5 solar activity cycles The large-scale behaviour of the green emission corona FeXIV 530.3 NM over the last 4.5 solar activity cycles

Apr 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994adspr..14...73s&link_type=abstract

Advances in Space Research, vol. 14, no. 4, p. (4)73-(4)76

Astronomy and Astrophysics

Astronomy

16

Emission Spectra, Solar Corona, Solar Cycles, Solar Rotation, Solar Spectra, Astronomical Observatories, Brightness, Fine Structure, Line Spectra, Solar Activity, Spectrum Analysis

Scientific paper

Existing coronagraphic measurements, obtained by the world-wide net of observatories, are used to characterize the large-scale variabilities and periodicities in the 530.3 nm emission corona over the period 1943-1991. Specifically, the time-latitude distribution of the coronal brightness is shown and in this connection the double maxima of the solar cycles, fine structure of the butterfly diagrams, N-S asymmetry and two modes -- rigid and differential -- of the coronal rotation are discussed.

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