Problems with models of the radiation belts
| dc.contributor.author | Daly, E.J. | |
| dc.contributor.author | Lemaire, J. | |
| dc.contributor.author | Heynderickx, D. | |
| dc.contributor.author | Rodgers, D.J. | |
| dc.date | 1996 | |
| dc.date.accessioned | 2017-05-23T10:04:27Z | |
| dc.date.available | 2017-05-23T10:04:27Z | |
| dc.identifier.uri | https://orfeo.belnet.be/handle/internal/5502 | |
| dc.description | The current standard models of the radiation-belt environment have many shortcomings, not the least of which is then- extreme age. Most of the data used for them were acquired in the 1%0's and early 1970's. Problems with the present models, and the ways in which data from more recent missions are being or can be used to create new models with improved functionality, are described. The phenomenology of the radiation belts, the effects on space systems, and geomagnetic coordinates and modeling are discussed. Errors found in present models, their functional limitations, and problems with their implementation and use are detailed. New modeling must address problems at low altitudes with the south Atlantic anomaly, east-west asymmetries and solar cycle variations, and at high altitudes with the highly dynamic electron environment. The important issues in space environment modeling from the point of view of usability and relationship with effects evaluation are presented. New sources of data are discussed. Future requirements in the data, models, and analysis tools areas are presented. | |
| dc.language | eng | |
| dc.title | Problems with models of the radiation belts | |
| dc.type | Article | |
| dc.subject.frascati | Physical sciences | |
| dc.audience | Scientific | |
| dc.source.title | IEEE Transactions on Nuclear Science | |
| dc.source.volume | 43 | |
| dc.source.issue | 2 | |
| dc.source.page | 403-415 | |
| Orfeo.peerreviewed | Yes | |
| dc.identifier.doi | 10.1109/23.490889 | |
| dc.identifier.scopus | 2-s2.0-0030130067 |
