Observations of CMEs without coronagraphs

H. Hudson (SPRC) and E. Cliver (AFRL)

With Yohkoh SXT and then SOHO/EIT and TRACE, we got our first good looks at motions of hot plasma in the low corona, both at the limb and on the disk. Thanks to this, we are learning a great deal about how CMEs begin. Best of all, we have the LASCO observations to "calibrate" these and many other relevant non-coronagraphic signatures.

What are we looking for?

Cartoons

List of Signatures

Does one scenario explain all CMEs?

Conclusions



Courtesy D. McKenzie and YPOP

Implosions are necessary