The Earth’s outer radiation belt often suffers from drastic changes in the electron fluxes. Since the electrons can be a potential threat to satellites, efforts have long been made to model and predict electron flux variations. In this paper, we describe a prediction model for the outer belt electrons that we have recently developed at Chungbuk National University. The model is based on a one-dimensional radial diffusion equation with observationally determined specifications of a few major ingredients in the following way. First, the boundary condition of the outer edge of the outer belt is specified by empirical functions that we determine using the THEMIS satellite observations of energetic electrons near the boundary. Second, the plasmapause locations are specified by empirical functions that we determine using the electron density data of THEMIS. Third, the model incorporates the local acceleration effect by chorus waves into the one-dimensional radial diffusion equation. We determine this chorus acceleration effect by first obtaining an empirical formula of chorus intensity as a function of drift shell parameter L*, incorporating it as a source term in the one-dimensional diffusion equation, and lastly calibrating the term to best agree with observations of a certain interval. We present a comparison of the model run results with and without the chorus acceleration effect, demonstrating that the chorus effect has been incorporated into the model to a reasonable degree.

1. INTRODUCTION
 2. PHYSICAL STRUCTURE OF THE MODEL
 3. EXAMPE OF MODEL RUNS
 4. SUMMARY AND FUTURE WORKS
 ACKNOWLEDGEMENTS
 REFERENCES

• Dae-Kyu Shin(Department of Astronomy and Space Science, Chungbuk National University)
• Dae-Young Lee(Department of Astronomy and Space Science, Chungbuk National University) Corresponding Author
• Jin-Hee Kim(Department of Astronomy and Space Science, Chungbuk National University)
• Jung-Hee Cho(Department of Astronomy and Space Science, Chungbuk National University)