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Prospects for Modeling and Forecasting SEP Events with ENLIL and SEPMOD

Published online by Cambridge University Press:  24 July 2018

J. G. Luhmann Open the ORCID record for J. G. Luhmann [Opens in a new window] ,
M. L. Mays ,
D. Odstrcil ,
Yan Li ,
H. Bain ,
C. O. Lee ,
C. M. S. Cohen ,
R. A. Mewaldt ,
R. A. Leske  and
Y. Futaana
J. G. Luhmann
Affiliation:
Space Sciences Laboratory, University of California, Berkeley, CA, USA email: [email protected]
M. L. Mays
Affiliation:
CCMC, NASA Goddard Space Flight Center, Greenbelt, MD, USA
D. Odstrcil
Affiliation:
George Mason University, Fairfax, VA, USA
Yan Li
Affiliation:
Space Sciences Laboratory, University of California, Berkeley, CA, USA email: [email protected]
H. Bain
Affiliation:
NOAA Space Weather Prediction Center, Boulder, CO, USA
C. O. Lee
Affiliation:
Space Sciences Laboratory, University of California, Berkeley, CA, USA email: [email protected]
C. M. S. Cohen
Affiliation:
California Institute of Technology, Pasadena, CA, USA
R. A. Mewaldt
Affiliation:
California Institute of Technology, Pasadena, CA, USA
R. A. Leske
Affiliation:
California Institute of Technology, Pasadena, CA, USA
Y. Futaana
Affiliation:
IRF, Kiruna, Sweden
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Abstract

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One view of major Solar Energetic Particle (SEP) events is that these (proton-dominated) fluxes are accelerated in heliospheric shock sources created by Interplanetary Coronal Mass Ejections (ICMEs), and then travel mainly along interplanetary magnetic field lines connecting the shock(s) to the observer(s). This places a particular emphasis on the role of the heliospheric conditions during the event, requiring a realistic description of the latter to interpret and/or model SEP events. The well-known ENLIL heliospheric simulation with cone model generated ICME shocks is used together with the SEPMOD particle event modeling scheme to demonstrate the value of applying these concepts at multiple inner heliosphere sites.

Keywords

Space weathersolar energetic particlesinterplanetary shocks
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 13 , Symposium S335: Space Weather of the Heliosphere: Processes and Forecasts , July 2017 , pp. 263 - 267
Copyright
Copyright © International Astronomical Union 2018 

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