CDS and SUMER observations of fine structure and dynamics of loops: Experience from HRTS

Details CDS and SUMER observations of fine structure and dynamics of loops: Experience from HRTS CDS and SUMER observations of fine structure and dynamics of loops: Experience from HRTS

Nov 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992esasp.348..155k&link_type=abstract

In ESA, Proceedings of the First SOHO Workshop: Coronal Streamers, Coronal Loops, and Coronal and Solar Wind Composition p 155-1

Astronomy and Astrophysics

Astronomy

1

Coronal Loops, Solar Atmosphere, Solar Corona, Spectrographs, Spectroscopic Telescopes, High Resolution, Regions, Solar Physics, Spaceborne Astronomy, Ultraviolet Spectrometers

Scientific paper

From observations with the High Resolution Telescope and Spectrograph (HRTS), it appears likely that the transition region in the solar atmosphere is characterized by an extreme fine structure, much smaller than one inch in size. The evidence from HRTS and other UV spectrometers for such small structure is discussed, and their structural and dynamical properties are outlined. The appropriate CDS (Coronal Diagnostic Spectrometer) and SUMER (Solar Ultraviolet Measurement of Emitted Radiation) observations needed to extend the knowledge of a finely structured transition region and corona are discussed.

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