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Proceedings Paper

Comparative analyses of the CSSS magnetic field calculation in the Univ. of California/San Diego tomographic solar wind model with in situ spacecraft observations
Author(s): Tamsen Dunn; P. Paul Hick; Bernard V. Jackson; Andrew Buffington; Xue Pu Zhao
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Paper Abstract

Our tomographic techniques developed over the last few years are based on kinematic models of the solar wind. This allows us to determine the large-scale three-dimensional extents of solar wind structures using interplanetary scintillation (IPS) observations and Thomson scattering brightness data in order to forecast their arrival at Earth in real time. We are specifically interested in a technique that can be combined with observations presently available from IPS velocity data and with observations which will become available from the Solar Mass Ejection Imager. In this paper, we introduce magnetic field projections from solar surface magnetogram data using the Stanford Current-Sheet Source Surface model at the source surface of our model and extrapolate the magnetic field out to and beyond Earth. The results are compared with in situ data. Real time projections of these data are available on our web site at: http://cassfos02.ucsd.edu/solar/forecast/index_v_n.html and http://cassfos02.ucsd.edu/solar/forecast/index_br_bt.html

Paper Details

Date Published: 4 February 2004
PDF: 8 pages
Proc. SPIE 5171, Telescopes and Instrumentation for Solar Astrophysics, (4 February 2004); doi: 10.1117/12.513759
Show Author Affiliations
Tamsen Dunn, Univ. of California/San Diego (United States)
P. Paul Hick, Univ. of California/San Diego (United States)
Bernard V. Jackson, Univ. of California/San Diego (United States)
Andrew Buffington, Univ. of California/San Diego (United States)
Xue Pu Zhao, Stanford Univ. (United States)


Published in SPIE Proceedings Vol. 5171:
Telescopes and Instrumentation for Solar Astrophysics
Silvano Fineschi; Mark A. Gummin, Editor(s)

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