Astronomy and Astrophysics – Astronomy
Scientific paper
May 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992esasp.344...91h&link_type=abstract
In ESA, Solar Physics and Astrophysics at Interferometric Resolution p 91-94 (SEE N93-10901 01-90)
Astronomy and Astrophysics
Astronomy
Emission Spectra, Plasma Acceleration, Solar Corona, Solar Wind, Stellar Mass Ejection, Chromosphere, High Resolution, Solar Atmosphere, Solar Prominences, Solar Spectra, Spaceborne Astronomy, Ultraviolet Spectra
Scientific paper
Requirements for detailed observation of ejecta and flows in the solar atmosphere are examined and the potential for observations of such phenomena using SIMURIS (Solar Interferometric Mission for Ultrahigh Resolution Imaging and Spectroscopy) are addressed. The solar atmosphere displays various ejection phenomena, with varying sizes, speeds, and characteristic time scales, presumably, resulting from various physical processes. These phenomena include the so called high velocity events detected in the transition region and the corona, chromospheric ejecta known as sprays and surges, and coronal mass ejecta, which include prominence eruptions. The salient observed features are discussed, and a brief description of the outstanding physical problems which govern the observational needs for each event type is given.
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