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The Coronal Diagnostic Spectrometer on SOHO

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Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 229))

Abstract

The solar extreme ultraviolet (EUV) spectrum, in the range 150–1200 Å, contains numerous emission lines whose intensities and profiles give us much valuable information for probing the upper chromosphere, transition region, and corona. The emissivities of these lines cover the temperature range 104 K to more than 106 K. Temperatures, densities, element abundances, flows, and turbulent velocities form the information that can be derived from analysis of line intensities and profiles.

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© 1998 Springer Science+Business Media Dordrecht

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Phillips, K.J.H., Harrison, R.A. (1998). The Coronal Diagnostic Spectrometer on SOHO. In: Watanabe, T., Kosugi, T., Sterling, A.C. (eds) Observational Plasma Astrophysics: Five Years of Yohkoh and Beyond. Astrophysics and Space Science Library, vol 229. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-5220-4_37

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  • DOI: https://doi.org/10.1007/978-94-011-5220-4_37

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-6198-8

  • Online ISBN: 978-94-011-5220-4

  • eBook Packages: Springer Book Archive

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