Registro completo de metadatos
| Campo DC | Valor | Lengua/Idioma |
|---|---|---|
| dc.provenance | CONICET | - |
| dc.creator | Dasso, Sergio Ricardo | - |
| dc.creator | Milano, L. J. | - |
| dc.creator | Matthaeus, W. H. | - |
| dc.creator | Smith, C. W. | - |
| dc.date | 2017-07-26T14:49:44Z | - |
| dc.date | 2017-07-26T14:49:44Z | - |
| dc.date | 2005-12 | - |
| dc.date | 2017-07-25T14:51:05Z | - |
| dc.date.accessioned | 2019-04-29T15:33:32Z | - |
| dc.date.available | 2019-04-29T15:33:32Z | - |
| dc.date.issued | 2005-12 | - |
| dc.identifier | Dasso, Sergio Ricardo; Milano, L. J.; Matthaeus, W. H.; Smith, C. W.; Anisotropy in fast and slow solar wind fluctuations; IOP Publishing; Astrophysical Journal; 635; 2; 12-2005; L181-L184 | - |
| dc.identifier | 0004-637X | - |
| dc.identifier | http://hdl.handle.net/11336/21326 | - |
| dc.identifier | CONICET Digital | - |
| dc.identifier | CONICET | - |
| dc.identifier.uri | http://rodna.bn.gov.ar:8080/jspui/handle/bnmm/296524 | - |
| dc.description | Using 5 years of spacecraft data from near Earth orbit, we investigate the correlation anisotropy of solar wind magnetohydrodynamic-scale fluctuations and show that the nature of the anisotropy differs in fast (>500 km/s) slow (<400 km/) streams. In particular, fast streams are relatively more dominated by fluctuations with wavevectors quasi-parallel to the local magnetic field, while slow streams, which appear to be more fully evolved turbulence, are more dominated by quasi-perpendicular fluctuation wavevectors. | - |
| dc.description | Fil: Dasso, Sergio Ricardo. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina | - |
| dc.description | Fil: Milano, L. J.. University of Delaware; Estados Unidos | - |
| dc.description | Fil: Matthaeus, W. H.. University of Delaware; Estados Unidos | - |
| dc.description | Fil: Smith, C. W.. University of New Hampshire; Estados Unidos | - |
| dc.format | application/pdf | - |
| dc.format | application/pdf | - |
| dc.language | eng | - |
| dc.publisher | IOP Publishing | - |
| dc.relation | info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1086/499559/meta | - |
| dc.relation | info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1086/499559 | - |
| dc.rights | info:eu-repo/semantics/restrictedAccess | - |
| dc.rights | https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ | - |
| dc.source | reponame:CONICET Digital (CONICET) | - |
| dc.source | instname:Consejo Nacional de Investigaciones Científicas y Técnicas | - |
| dc.source | instacron:CONICET | - |
| dc.source.uri | http://hdl.handle.net/11336/21326 | - |
| dc.subject | solar wind | - |
| dc.subject | turbulence | - |
| dc.subject | cosmic rays | - |
| dc.subject | Astronomía | - |
| dc.subject | Ciencias Físicas | - |
| dc.subject | CIENCIAS NATURALES Y EXACTAS | - |
| dc.title | Anisotropy in fast and slow solar wind fluctuations | - |
| dc.type | info:eu-repo/semantics/article | - |
| dc.type | info:eu-repo/semantics/publishedVersion | - |
| dc.type | info:ar-repo/semantics/articulo | - |
| Aparece en las colecciones: | CONICET | |
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