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Read Full Article (file size: 412505 bytes) Cited by
SPACE WEATHER,
VOL. 5,
S11003,
doi:10.1029/2006SW000296,
2007
Solar wind parameters for magnetospheric magnetic field modeling
Z. Qin
Department of Physics and Astronomy, Dartmouth College, Hanover, New Hampshire, USA
R. E. Denton
Department of Physics and Astronomy, Dartmouth College, Hanover, New Hampshire, USA
N. A. Tsyganenko
USRA, NASA Goddard Space Flight Center, Greenbelt, Maryland, USA
S. Wolf
Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan, USA
Abstract
Magnetospheric magnetic field models are crucial for many space weather applications. However, the latest empirical models
require solar wind and IMF data, which are not always available. Data gaps are especially common for times before the launch
of the WIND spacecraft at the end of 1994, but even after then there are data gaps. We present a method to interpolate the
solar wind characteristics across data gaps and to evaluate the W parameters needed for the TS05 model (Tsyganenko and Sitnov, 2005). Within some distance from the edge of a data gap, the
solar wind parameters from our method yield a better estimate of the observed magnetic field than that which could be found
using average values of the parameters. Deep within data gaps (far from measured values), the interpolated parameters are
reasonable, or typical values, no better or worse than average values. We have created a database of hourly data with solar
wind characteristics, G, and W parameters from 1963 to 31 May 2007, which is sufficient for use in all the Tsyganenko models, including the latest TS05
model. Our comparisons of the model and observed magnetic field at geosynchronous orbit give an estimate of the error in the
model field as a function of status parameters defined by the interpolation scheme. We also show that the model field is on
average just as accurate using the hourly data as that based on 5 min data (at least at geosynchronous orbit).
Received 12
October
2006;
accepted 12
August
2007;
published 22
November
2007.
Keywords: magnetic field models;
solar wind parameters.
Index Terms: 2740 Magnetospheric Physics: Magnetospheric configuration and dynamics; 2753 Magnetospheric Physics: Numerical modeling; 7833 Space Plasma Physics: Mathematical and numerical techniques (0500, 3200); 7959 Space Weather: Models.
Read Full Article (file size: 412505 bytes) Cited by
Citation: Qin, Z., R. E. Denton, N. A. Tsyganenko, and S. Wolf
(2007),
Solar wind parameters for magnetospheric magnetic field modeling,
Space Weather,
5,
S11003,
doi:10.1029/2006SW000296.
Copyright 2007 by the American Geophysical Union.
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