YOHKOH observations of the solar corona

Details YOHKOH observations of the solar corona YOHKOH observations of the solar corona

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997adspr..19.1839c&link_type=abstract

Advances in Space Research, vol. 19, p. 1839

Other

5

Solar Corona, Coronal Mass Ejection, Solar X-Rays, X Ray Telescopes, Solar Activity, Plasma Temperature, Solar Observatories, Spectral Signatures, Emission Spectra

Scientific paper

X-ray signatures for coronal mass ejection (CME) events involving the detection of reduced X-ray intensities in the corona have been developed on the basis of Yohkoh soft X-ray telescope data. These CME observations indicate that while the active region emission correlates well with other activity indicators, there is no strong connection with plasma temperature.

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