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dc.contributor.authorHenriksen, K.
dc.contributor.authorShumilov, O.I.
dc.contributor.authorKasatkina, E.A.
dc.contributor.authorVashenyuk, E.V.
dc.date.accessioned2007-01-24T09:51:10Z
dc.date.available2007-01-24T09:51:10Z
dc.date.issued1996
dc.description.abstractThe lidar measurements at Verhnetulomski observatory (68.6¡N, 31.8¡E) at Kola peninsula detected a considerable increase of stratospheric aerosol concentration after the solar proton event of GLE (ground level event) type on the 16/02/84. This increase was located at precisely the same altitude range where the energetic solar protons lost their energy in the atmosphere. The aerosol layer formed precipitated quickly (1Ð2 km per day) during 18, 19, and 20 February 1984, and the increase of R(H) (backscattering ratio) at 17 km altitude reached 40% on 20/02/84. We present the model calculation of CN (condensation nuclei) altitude distribution on the basis of an ion-nucleation mechanism, taking into account the experimental energy distribution of incident solar protons. The meteorological situation during the event was also investigated.en
dc.format.extent215885 bytes
dc.format.mimetypeapplication/pdf
dc.identifier.issn1432-0576 (elektronisk)
dc.identifier.urihttps://hdl.handle.net/10037/554
dc.identifier.urnURN:NBN:no-uit_munin_381
dc.language.isoengen
dc.publisherEuropean Geophysical Societyen
dc.relation.ispartofseriesAnnales Geophysicae 14(1996), pp 1119-1123en
dc.rights.accessRightsopenAccess
dc.subjectVDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Rom- og plasmafysikk: 437en
dc.subjectVDP::Matematikk og Naturvitenskap: 400::Geofag: 450::Meteorologi: 453en
dc.titleEnhancement of stratospheric aerosols after solar proton event.en
dc.typeJournal articleen
dc.typeTidsskriftartikkelno


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