IPS Observations of Flare-Generated Disturbances

Takashi Watanabe
1980 Symposium - International astronomical union  
Dynamical behaviour of a flare-generated disturbance can be followed by IPS observations through a comparison between the IPS observations and a model of the disturbance. The highly turbulent post-shock plasma can be attributed to the contact surface of the disturbance. Two examples of IPS observations of flare-generated disturbances will be discussed.
doi:10.1017/s0074180900067929 fatcat:tu7qmb4zjbhvjorbekfaz2auue