Real-Time Dst Model

(What is Dst?)

This data is updated 1/2-hourly at the 0 and 30 minutes past the hour. The purpose of this exercise is to demonstrate that real time Solar Wind data can be used to produce a simple model of Dst.
These data are NOT for publication use.

 The handling of ACE data gaps is incomplete.Use this data at your own risk.


General Description

The original ACE resolution is 1 minute. Propagation is, for the moment, purely ballistic, with the spacecraft assumed to be exactly at the L1 point.

Dst is a measure of the terrestrial ring current, given in nT.

Our Model works as follows:

Dst(t) = Dst0(t) + b*(Pdyn)1/2 + d0
dDst0/dt = Q*(VBs-E0) - Dst0/t
t ~ exp[1/(a'+VBs)]

Dst0 is the time integrated influence of VBs, the induced electric field Ey. VBs is given in mV/m.

E0 is a threshold value for VBs, below which there is no injection of energy to the ring current.

 Pdyn is the Solar Wind Dynamic Pressure, in nPa.  Dst0 is corrected for the motion of the magnetopause currents, which are influenced by  Pdyn

 The final Dst is what we expect to be measured.

We initialize our model using the Kyoto Near Real-Time Dst(t0), thereafter ACE solar wind data and the equations above are used to calculate running estimates of Dst.


Want to Find Out More?

An explanation and evaluation of the real-time performance of this model is provided in From Research To Real-Time: Modeling and Forecasting the Ring Current [MS PowerPoint] [gifs]

This model is described in greater detail in:

 Other Space Weather Forecasts 


Prepared by Paul O'Brien, tpoiii@igpp.ucla.edu

Space Science Center
Institute of Geophysics and Planetary Physics
University of California, Los Angeles