%0 Journal Article
%@holdercode {isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S}
%@nexthigherunit 8JMKD3MGPCW/3EU29DP
%@resumeid 8JMKD3MGP5W/3C9JH3D
%@archivingpolicy denypublisher denyfinaldraft24
%@usergroup administrator
%@usergroup banon
%@usergroup simone
%3 foreshock.pdf
%X Foreshock and magnetosheath waves in Uranus and Neptune magnetospheres are studied in this work with wavelet analysis. In order to conduct this study, Voyager-2 magnetometer 3-s averaged data are used. The Morlet wavelet transform is applied to the magnetic field vector data. Waves present in the magnetosheath and foreshock regions are highly non-stationary, showing large amplitude variations. It was found that the dominant periods of these waves are longer than the H+ cyclotron period. Overall, high frequency waves are seen near the bow shock crossing and low frequency oscillations near the magnetopause crossing. It can be concluded that non-stationary foreshock and magnetosheath planetary waves can be well characterized with wavelet analysis.
%@mirrorrepository sid.inpe.br/mtc-m19@80/2009/08.21.17.02.53
%8 Nov.
%N 9
%T Foreshock and magnetosheath waves at Uranus and Neptune studied with wavelet analysis
%@secondarytype PRE PI
%K Foreshock waves, Magnetosheath waves, Uranus magnetosphere, Neptune magnetosphere, Solar wind, Wavelet analysis.
%@group DGE-CEA-INPE-MCT-BR
%@secondarykey INPE--PRE/
%@secondarymark B3_CIÊNCIAS_BIOLÓGICAS_I B1_ENGENHARIAS_III B2_ENGENHARIAS_IV B1_GEOCIÊNCIAS A2_INTERDISCIPLINAR
%@issn 0273-1177
%2 sid.inpe.br/mtc-m19@80/2009/12.09.18.33.37
%@affiliation Instituto Nacional de Pesquisas Espaciais (INPE)
%B Advances in Space Research
%P 1030-1037
%4 sid.inpe.br/mtc-m19@80/2009/12.09.18.33
%D 2009
%V 44
%@doi 10.1016/j.asr.2009.05.024
%A Echer, Ezequiel,
%@dissemination WEBSCI; PORTALCAPES; MGA; COMPENDEX.
%@area CEA