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ESA SEPEM Project: peak flux and fluence model

ESA SEPEM Project: peak flux and fluence model
ESA SEPEM Project: peak flux and fluence model
A new modelling methodology for the prediction of the solar proton environment a 1 AU developed as part of the Solar Energetic Particle Environment (SEPEM) Project for the European Space Agency (ESA) is presented. This new method named Virtual Timelines is applied to the SEPEM Reference Event List derived from a long flux time series of space-based measurements to produce the SEPEM model for proton peak flux and fluence at 1 AU. There are several new components including the use of the Le ?vy distribution for time distributions and the accounting for the non-point-like nature of SEP events.
0018-9499
1066-1077
Gabriel, S.B.
ac76976d-74fd-40a0-808d-c9f68a38f259
Jiggens, P.T.A.
04569b9f-858b-44b1-a6bd-4b316e1164d6
Heynderickx, D.
3fb1b586-1e50-482a-8cd9-cb76c15123ff
Crosby, N.
b0077a31-a90f-4f4a-a52e-0c2ba0843753
Glover, A.
31dd7ea2-17b9-47c4-866f-4be9b9a4a991
Hilgers, A.
3bba8539-449a-4bdd-bf01-ba16e2025b27
Gabriel, S.B.
ac76976d-74fd-40a0-808d-c9f68a38f259
Jiggens, P.T.A.
04569b9f-858b-44b1-a6bd-4b316e1164d6
Heynderickx, D.
3fb1b586-1e50-482a-8cd9-cb76c15123ff
Crosby, N.
b0077a31-a90f-4f4a-a52e-0c2ba0843753
Glover, A.
31dd7ea2-17b9-47c4-866f-4be9b9a4a991
Hilgers, A.
3bba8539-449a-4bdd-bf01-ba16e2025b27

Gabriel, S.B., Jiggens, P.T.A., Heynderickx, D., Crosby, N., Glover, A. and Hilgers, A. (2012) ESA SEPEM Project: peak flux and fluence model. IEEE Transactions on Nuclear Science, 59 (4), 1066-1077. (doi:10.1109/TNS.2012.2198242).

Record type: Article

Abstract

A new modelling methodology for the prediction of the solar proton environment a 1 AU developed as part of the Solar Energetic Particle Environment (SEPEM) Project for the European Space Agency (ESA) is presented. This new method named Virtual Timelines is applied to the SEPEM Reference Event List derived from a long flux time series of space-based measurements to produce the SEPEM model for proton peak flux and fluence at 1 AU. There are several new components including the use of the Le ?vy distribution for time distributions and the accounting for the non-point-like nature of SEP events.

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More information

Published date: August 2012
Organisations: EEE

Identifiers

Local EPrints ID: 339324
URI: http://eprints.soton.ac.uk/id/eprint/339324
ISSN: 0018-9499
PURE UUID: 344d65f0-90b2-4bfb-bcad-0a9104ba276a

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Date deposited: 28 May 2012 15:20
Last modified: 14 Mar 2024 11:13

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Contributors

Author: S.B. Gabriel
Author: P.T.A. Jiggens
Author: D. Heynderickx
Author: N. Crosby
Author: A. Glover
Author: A. Hilgers

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