Relations between the photospheric magnetic field and the emission from the outer atmospheres of cool stars. II - The C IV 1550 A doublet

Astronomy and Astrophysics – Astrophysics

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Cool Stars, Magnetic Flux, Photosphere, Solar Activity Effects, Solar Magnetic Field, Stellar Activity, Ultraviolet Spectra, Exosat Satellite, Flux Density, Heao 2, Iue, Optical Thickness

Scientific paper

Solar and stellar data are used to determine the relationship between C IV 1548 + 1551 A and magnetic flux densities. C IV SMM-UVSP spectroheliograms of solar quiet regions and plages are analyzed. Typical distribution functions of C IV flux densities over both quiet and active solar regions are presented. The C IV emission is shown to be dependent on magnetic flux density.

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