On the filling factor of emitting material in the upper atmosphere of ε Eri (K2 V)

S.A. Sim, C. Jordan

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9 Citations (Scopus)

Abstract

The emission measure distribution in the upper transition region and corona of e Eri is derived from observed emission-line fluxes. Theoretical emission measure distributions are calculated assuming that the radiation losses are balanced by the net conductive flux. We discuss how the area factor of the emitting regions as a function of temperature can be derived from a comparison between these emission measure distributions. It is found that the filling factor varies from ~0.2 in the mid-transition region to ~1.0 in the inner corona. The sensitivity of these results to the adopted ion fractions, the iron abundance and other parameters is discussed. The area factors found are qualitatively similar to the observed structure of the solar atmosphere, and can be used to constrain two-component models of the chromosphere. Given further observations, the method could be applied to investigate the trends in filling factors with indicators of stellar activity.
Original languageEnglish
Pages (from-to)846-854
Number of pages9
JournalMonthly Notices of the Royal Astronomical Society
Volume346
Issue number3
DOIs
Publication statusPublished - 11 Dec 2003

Bibliographical note

Copyright 2012 Elsevier B.V., All rights reserved.

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