Coronal index of solar activity 7, years 1988-1991

Details Coronal index of solar activity 7, years 1988-1991 Coronal index of solar activity 7, years 1988-1991

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994soph..152..487r&link_type=abstract

Solar Physics, vol. 152, no. 2, p. 487-495

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Applications

25

Applications Of Mathematics, Correlation, Emission Spectra, Iron, Line Spectra, Radio Astronomy, Solar Activity, Solar Corona, Stellar Models, Visible Spectrum, X Ray Astronomy, Astronomical Photometry, Coronagraphs, Emissivity, Fourier Analysis, Irradiance, Solar Limb, Solar Magnetic Field

Scientific paper

A brief description is given of the coronal index of solar activity (CI) derived from ground-based observations of the green coronal line 530.3 nm Fe XIV and its computation. The final data of CI are presented in graphical form over the period 1988-1991. The maximum of CI coincide with the Wolf number in cycle 22, and no second maximum, sometimes seen two years after the first one, was observed in this cycle.

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