Halo CMEs in the Ultraviolet

Details Halo CMEs in the Ultraviolet Halo CMEs in the Ultraviolet

May 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aas...200.3707r&link_type=abstract

American Astronomical Society, 200th AAS Meeting, #37.07; Bulletin of the American Astronomical Society, Vol. 34, p.695

Astronomy and Astrophysics

Astronomy

Scientific paper

Halo CMEs are especially important for connecting remote sensing observations with in situ measurements, as well as for Space Weather. However, analysis of coronagraphic observations of halo CMEs is complicated by relatively severe projection effects. We discuss the use of Doppler shifts to constrain CME structure and evolution along the line-of-sight, and we discuss the excitation of UV emission lines at high velocities and large heights above the Sun. This work was supported by NASA Grant NAG5-11420.

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