What's needed in the UV and EUV

Details What's needed in the UV and EUV What's needed in the UV and EUV

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987nascp2483...37d&link_type=abstract

In NASA-Goddard Space Flight Center, Theoretical Problems in High Resolution Solar Physics, 2 p 37-54 (SEE N88-11609 02-92)

Physics

7

Extreme Ultraviolet Radiation, Solar Atmosphere, Spatial Resolution, Spectral Resolution, Ultraviolet Spectroscopy, Plasma Diagnostics, Solar Corona, Solar Physics, Solar Temperature

Scientific paper

High spectral and spatial resolution UV and EUV spectroscopy is discussed with emphasis on the spectroscopic observations that are required in order to increase our understanding of the physics of the lower transition region. The properties of the lower transition region are reviewed, and the available lower transition region plasma diagnostics are reviewed for the wavelength range between about 1150 and 2000 Å. One important conclusion is that comprehensive spectroscopic coverage over a rather broad temperature range is necessary in order to observe satisfactorily small transition region structures. This is illustrated by two examples from the recent NRL Spacelab 2 HRTS experiment.

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