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Fisher, George H. - Space Sciences Laboratory, University of California at Berkeley
Coronal Heating in Active Regions As a Function of Global Magnetic Variables
The Origin of Twisted Magnetic Fields
An Observational Test of Transition Region Lines as a Pressure Gauge
Simultaneous SOHO and Yohkoh Observations of a Small Solar Active Region
The Origin of Magnetic Fields
MULTIMODE KINK INSTABILITY AS A MECHANISM FOR ffiSPOT FORMATION
The Origin and Role of Twist in Active Regions G. H. Fisher
Twisted flux tubes and how they get that way Dana Longcope, 1 Mark Linton, 2 Alexei Pevtsov, 1 George Fisher, 2 and Isaac Klapper 3
The Solar Dynamo and Emerging Flux G. H. Fisher (fisher@ssl.berkeley.edu)
Starspots: The Zebra Effect Bjrn R. Pettersen
THE DYNAMICS OF MAGNETIC FLUX TUBES IN THE SOLAR CONVECTION ZONE
Models of Rising Active Region Flux Tubes George H. Fisher
The 3D MHD Simulation of Flux Tube Dynamics
THE ASTROPHYSICAL JOURNAL, 514:472483, 1999 March 20 1999. The American Astronomical Society. All rights reserved. Printed in U.S.A.(
