dc.contributor.author | Henriksen, K. | |
dc.contributor.author | Shumilov, O.I. | |
dc.contributor.author | Kasatkina, E.A. | |
dc.contributor.author | Vashenyuk, E.V. | |
dc.date.accessioned | 2007-01-24T09:51:10Z | |
dc.date.available | 2007-01-24T09:51:10Z | |
dc.date.issued | 1996 | |
dc.description.abstract | The 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.extent | 215885 bytes | |
dc.format.mimetype | application/pdf | |
dc.identifier.issn | 1432-0576 (elektronisk) | |
dc.identifier.uri | https://hdl.handle.net/10037/554 | |
dc.identifier.urn | URN:NBN:no-uit_munin_381 | |
dc.language.iso | eng | en |
dc.publisher | European Geophysical Society | en |
dc.relation.ispartofseries | Annales Geophysicae 14(1996), pp 1119-1123 | en |
dc.rights.accessRights | openAccess | |
dc.subject | VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Rom- og plasmafysikk: 437 | en |
dc.subject | VDP::Matematikk og Naturvitenskap: 400::Geofag: 450::Meteorologi: 453 | en |
dc.title | Enhancement of stratospheric aerosols after solar proton event. | en |
dc.type | Journal article | en |
dc.type | Tidsskriftartikkel | no |