Registro completo de metadatos
| Campo DC | Valor | Lengua/Idioma |
|---|---|---|
| dc.creator | Matthaeus, W. H. | - |
| dc.creator | Weygand, J. M. | - |
| dc.creator | Chuychai, P. | - |
| dc.creator | Dasso, Sergio Ricardo | - |
| dc.creator | Smith, C. W. | - |
| dc.creator | Kivelson, M. G. | - |
| dc.date | 2017-07-17T18:35:56Z | - |
| dc.date | 2017-07-17T18:35:56Z | - |
| dc.date | 2008-12 | - |
| dc.date | 2017-07-17T13:32:52Z | - |
| dc.date.accessioned | 2019-04-29T15:40:22Z | - |
| dc.date.available | 2019-04-29T15:40:22Z | - |
| dc.date.issued | 2017-07-17T18:35:56Z | - |
| dc.date.issued | 2017-07-17T18:35:56Z | - |
| dc.date.issued | 2008-12 | - |
| dc.date.issued | 2017-07-17T13:32:52Z | - |
| dc.identifier | Matthaeus, W. H.; Weygand, J. M.; Chuychai, P.; Dasso, Sergio Ricardo; Smith, C. W.; et al.; Interplanetary magnetic Taylor microscale and implications for plasma dissipation; IOP Publishing; Astrophysical Journal; 678; 2; 12-2008; 1-4, L141 | - |
| dc.identifier | 0004-637X | - |
| dc.identifier | http://hdl.handle.net/11336/20714 | - |
| dc.identifier | CONICET Digital | - |
| dc.identifier | CONICET | - |
| dc.identifier.uri | http://rodna.bn.gov.ar:8080/jspui/handle/bnmm/299125 | - |
| dc.description | The Taylor microscale, a measure of mean square spatial derivatives, is evaluated for interplanetary magnetic field fluctuations from single- and multiple-point data using Cluster and ACE spacecraft data. The Taylor scale is compared to the measured inner scale, which for hydrodynamics would correspond to the Kolmogorov scale. The results are not consistent with dissipation of the hydrodynamic type, and indicate that solar wind dissipation involves kinetic plasma physics at both proton and electron scales. | - |
| dc.description | Fil: Matthaeus, W. H.. University of Delaware; Estados Unidos | - |
| dc.description | Fil: Weygand, J. M.. University of California; Estados Unidos | - |
| dc.description | Fil: Chuychai, P.. University of Delaware; Estados Unidos | - |
| 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: Smith, C. W.. University of New Hampshire; Estados Unidos | - |
| dc.description | Fil: Kivelson, M. G.. University of California; 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/10.1086/588525 | - |
| dc.relation | info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1086/588525 | - |
| 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.subject | Astronomía | - |
| dc.subject | Ciencias Físicas | - |
| dc.subject | CIENCIAS NATURALES Y EXACTAS | - |
| dc.title | Interplanetary magnetic Taylor microscale and implications for plasma dissipation | - |
| 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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