EUV Spectroscopy as a Plasma Diagnostic

Details EUV Spectroscopy as a Plasma Diagnostic EUV Spectroscopy as a Plasma Diagnostic

Sep 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ssrv...65..289d&link_type=abstract

Space Science Reviews, Volume 65, Issue 3-4, pp. 289-316

Physics

23

Scientific paper

The EUV wavelength regions is rich in emission lines from the transition region and the corona. Spectroscopic techniques have been used extensively to determine the physical conditions in the solar atmosphere for such diverse phenomena as coronal holes, active regions, sunspots, flares, etc. The diagnostics and dynamics of plasmas, both homogeneous and inhomogeneous plasmas, are reviewed. The future projects such as the CDS and SUMER instruments on SOHO have been discussed as they cover EUV wavelength region and will provide a wealth of observational data with excellent spatial, spectral, and temporal resolution.

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