G. Lawrence

发表

Cone model for halo CMEs: Application to space weather forecasting

L. Ofman, H. Xie, G. Lawrence, 2004 .

Low-density anomalies and sub-Alfvénic solar wind

K. Ogilvie, W. Farrell, M. Goldstein, 2005 .

Plasma depletion layer model for low Alfvén Mach number: Comparison with ISEE observations

R. Elphic, C. Farrugia, H. Biernat, 1997 .

Dynamical and Physical Properties of a Post-Coronal Mass Ejection Current Sheet

J. Raymond, A. Fludra, Y. Ko, 2003 .

Rapid Acceleration of a Coronal Mass Ejection in the Low Corona and Implications for Propagation

P. Gallagher, B. Dennis, G. Lawrence, 2003 .

Are CME “interactions” really important for accelerating major solar energetic particle events?

D. Haggerty, A. Szabo, T. Kucera, 2003 .

Wind and ACE observations during the great flow of 1–4 May 1998: Relation to solar activity and implications for the magnetosphere

J. Dwyer, L. Burlaga, H. Matsui, 2002 .

Power to the magnetosphere: May 4, 1998

M. Freeman, L. Burlaga, H. Matsui, 2003 .

Interaction between coronal mass ejections and the solar wind

M. Bisi, R. Fallows, A. Breen, 2007 .