The solar stellar connection in the far ultraviolet

Details The solar stellar connection in the far ultraviolet The solar stellar connection in the far ultraviolet

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984nascp2349..437b&link_type=abstract

In NASA. Goddard Space Flight Center Future of Ultraviolet Astronomy Based on Six Years of IUE Res. p 437-440 (SEE N85-20961 1

Astronomy and Astrophysics

Astronomy

3

Far Ultraviolet Radiation, Iue, Main Sequence Stars, Stellar Atmospheres, Stellar Flares, Abundance, Algorithms, Data Smoothing, Spatial Resolution, Spectral Resolution

Scientific paper

The authors compare the far-ultraviolet "activity" of solar-type stars, as measured with the IUE, to that of the Sun, as measured by the Solar Irradiance Monitor of the Solar Mesosphere Explorer. The goal of the study is to explore the relationships between the "ultraviolet activity" at different levels of the atmospheres of solar type stars. Secondary goals are to establish the strength of the solar ultraviolet activity within the class of solar-type stars, and to examine the amplitudes of rotational modulations of the solar emission lines during the declining portion of the current sunspot cycle. A unique aspect of the study is that the spectral resolution of the SME instrument (7.5 Å) compares very favorably with that of the low dispersion model of the IUE (5 Å).

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