Multi-wavelength Signatures of Coronal Mass Ejection

Details Multi-wavelength Signatures of Coronal Mass Ejection Multi-wavelength Signatures of Coronal Mass Ejection

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999spro.proc..207g&link_type=abstract

Solar Physics with Radio Observations, Proceedings of the Nobeyama Symposium, held in Kiyosato, Japan, Oct. 27-30, 1998, Edited

Physics

3

Scientific paper

We report on the near-surface and outer coronal manifestations of the 1998 January 25 coronal mass ejection (CME) using white light, EUV, X-ray and hectometric radio data which reveal the three dimensional structure and long term evolution of the CME. We find that (i) the substructures of the CME (prominence core, cavity, frontal structure and the arcade formation) are clearly observed in X-ray and EUV wavelengths. (ii) The filament heats up early on and is observed as a backbone in X-rays. (iii) The filament also expands considerably as it erupts. (iv) The CME is observed through direct leading edge signature as well as through dimming process in X-rays and in EUV.

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