A Comparison of CME-associated atmospheric waves observed in coronal (19.5 nm) and chromospheric (He I 1083 nm and H-alpha 656 nm) lines

Details A Comparison of CME-associated atmospheric waves observed in coronal (19.5 nm) and chromospheric (He I 1083 nm and H-alpha 656 nm) lines A Comparison of CME-associated atmospheric waves observed in coronal (19.5 nm) and chromospheric (He I 1083 nm and H-alpha 656 nm) lines

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agufmsh12b0746g&link_type=abstract

American Geophysical Union, Fall Meeting 2001, abstract #SH12B-0746

Physics

7507 Chromosphere, 7509 Corona, 7513 Coronal Mass Ejections, 7519 Flares

Scientific paper

Coronal Mass Ejections (CMEs) are frequently associated with wave phenomena observed in the corona, and sometimes with wave phenomena observed in the chromosphere. We have studied CME-associated waves observed in both coronal (19.5 nm) and chromospheric (He I 1083 nm and H-alpha 656 nm) lines. Comparison of the coronal and chromospheric signatures allows us to understand better the relationship between the two wave phenomena.

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