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dc.contributor.authorLemaire, J.F.
dc.contributor.authorSinger, S.F.
dc.date2012
dc.date.accessioned2016-03-29T10:07:37Z
dc.date.available2016-03-29T10:07:37Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/3008
dc.descriptionDuring geomagnetic field reversals the radiation belt high-energy proton populations become depleted. Their energy spectra become softer, with the trapped particles of highest energies being lost first, and eventually recovering after a field reversal. The radiation belts rebuild in a dynamical way with the energy spectra flattening on the average during the course of many millennia, but without ever reaching complete steady state equilibrium between successive geomagnetic storm events determined by southward turnings of the IMF orientation. Considering that the entry of galactic cosmic rays and the solar energetic particles with energies above a given threshold are strongly controlled by the intensity of the northward component of the interplanetary magnetic field, we speculate that at earlier epochs when the geomagnetic dipole was reversed, the entry of these energetic particles into the geomagnetic field was facilitated when the interplanetary magnetic field was directed northward. Unlike in other complementary work where intensive numerical simulations have been used, our demonstration is based on a simple analytical extension of Stormer's theory. The access of GCR and SEP beyond geomagnetic cut-off latitudes is enhanced during epochs when the Earth's magnetic dipole is reduced, as already demonstrated earlier.
dc.languageeng
dc.publisherAmerican Geophysical Union
dc.titleWhat happens when the geomagnetic field reverses?
dc.typeBook chapter
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleDynamics of the Earth's Radiation Belts and Inner Magnetosphere
dc.source.volume199
dc.source.page355-363
Orfeo.peerreviewedYes
dc.identifier.doi10.1029/2012GM001307
dc.identifier.scopus2-s2.0-84899567202
dc.source.editorSummers, D.
dc.source.editorMann, I.R.
dc.source.editorSchulz, M.
dc.source.editorBaker, D.N.


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