Magnetic Source Region Characteristics Influencing the Velocity of Solar Eruptions in the Corona
Bernhard Kliem1, Georgios Chintzoglou2, Dr. Tibor Torok3, Jie Zhang4 and Cooper Downs3, (1)University of Potsdam, Institute of Physics and Astronomy, Potsdam, Germany, (2)Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States, (3)Predictive Science Inc., San Diego, United States, (4)George Mason University, Department of Physics and Astronomy, Fairfax, VA, United States
