Physics
Scientific paper
Dec 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agufmsh31a0701d&link_type=abstract
American Geophysical Union, Fall Meeting 2001, abstract #SH31A-0701
Physics
2134 Interplanetary Magnetic Fields, 2164 Solar Wind Plasma, 7524 Magnetic Fields
Scientific paper
Our time-dependent tomographic technique developed over the last few years provides a kinematic model of the solar wind. The model, which has one-day time steps, allows us to determine the large-scale three dimensional extent of solar disturbances and to forecast their arrival at Earth in real-time. We introduce magnetic field calculations from the Stanford Current-Sheet Source Surface model (Zhao and Hoeksema, 1995) at the source surface of our kinematic model and extrapolate the magnetic field out beyond Earth. We show an animated version of the convected magnetic field, and compare results with in situ data near Earth. We wish to thank Dr. XuePu Zhao for providing software and input data for the Stanford Current-Sheet Source Surface model. This work is supported by AFOSR contract F49620-01-1-0360. References: Zhao, X. and J.T. Hoeksema, Prediction of the interplanetary magnetic field strength, J. Geophys. Res. 100, 19, 1995.
Buffington Andrew
Dunn Tyler
Hick Pierre P.
Jackson Bernard V.
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