American Geophysical Union Become an AGU Member
Subscribe to AGU Journals		 AGU Home AGU Publications

Read Full Article (file size: 1072315 bytes)    Cited by

JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 107, NO. A12, 1472, doi:10.1029/2001JA007532, 2002

A new model for the prediction of Dst on the basis of the solar wind

M. Temerin

Space Sciences Laboratory, University of California, Berkeley, California, USA


Xinlin Li

Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, Colorado, USA


Abstract

An explicit model for predicting Dst based on solar wind data for the years 1995–1999 gives a good fit with a prediction efficiency of 88%, a linear correlation coefficient between the Dst index and the model of 0.94, and a RMS error of 6.4 nT. The same model applied to the first half of 2000 gave a prediction efficiency of 91%, a linear correlation coefficient of 0.95, and a RMS error of 7.9 nT. The modeled Dst is a sum of three terms that have growth and decay, a dynamic pressure term, an interplanetary magnetic field term, and some offset terms. The main innovations are that the decay terms have different time constants ranging from 5 days to 1 hour and that all the terms except the offsets depend on the angle of the Earth's dipole with respect to the solar wind velocity. This result shows that the magnetosphere is highly predictable and that chaotic behavior within the magnetosphere has little influence on the large-scale currents that determine Dst.

Published 24 December 2002.

Index Terms: 2788 Magnetospheric Physics: Storms and substorms; 2778 Magnetospheric Physics: Ring current; 2722 Magnetospheric Physics: Forecasting.

Read Full Article (file size: 1072315 bytes)    Cited by

Citation: Temerin, M., and X. Li (2002), A new model for the prediction of Dst on the basis of the solar wind, J. Geophys. Res., 107(A12), 1472, doi:10.1029/2001JA007532.