The solar wind angular momentum and energy carried by the interplanetary magnetic field
Solutions already found by one of the authors with a two-region model of the solar coronal expansion are used to analyze the transport of angular momentum and energy by the interplanetary magnetic field. In agreement with observations, it is predicted that the interplanetary magnetic field plays an...
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| Formato: | Capítulo de libro |
| Lenguaje: | Inglés |
| Publicado: |
Kluwer Academic Publishers
1995
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| Acceso en línea: | Registro en Scopus DOI Handle Registro en la Biblioteca Digital |
| Aporte de: | Registro referencial: Solicitar el recurso aquí |
| LEADER | 04566caa a22004937a 4500 | ||
|---|---|---|---|
| 001 | PAPER-3739 | ||
| 003 | AR-BaUEN | ||
| 005 | 20230518203312.0 | ||
| 008 | 190411s1995 xx ||||fo|||| 00| 0 eng|d | ||
| 024 | 7 | |2 scopus |a 2-s2.0-0542362693 | |
| 040 | |a Scopus |b spa |c AR-BaUEN |d AR-BaUEN | ||
| 100 | 1 | |a Alexander, P. | |
| 245 | 1 | 4 | |a The solar wind angular momentum and energy carried by the interplanetary magnetic field |
| 260 | |b Kluwer Academic Publishers |c 1995 | ||
| 270 | 1 | 0 | |m Alexander, P.; Departamento de Física, Facultad de Ciencias Exactas y Naturales, Universidad de Buenos AiresArgentina |
| 506 | |2 openaire |e Política editorial | ||
| 504 | |a Acuña, M., Whang, Y.C., A two-region model of the solar wind including azimuthal velocity (1976) The Astrophysical Journal, 203, p. 720 | ||
| 504 | |a Alexander, P., (1993) Astrophys. J., 414, p. 372. , Paper I | ||
| 504 | |a Barnes, A., Acceleration of the Solar Wind by the Interplanetary Magnetic Field (1974) The Astrophysical Journal, 188, p. 645 | ||
| 504 | |a Hollweg, J.V., Alfvén waves in the solar wind: Wave pressure, poynting flux, and angular momentum (1973) Journal of Geophysical Research, 78, p. 3643 | ||
| 504 | |a Hundhausen, A.J., Bame, S.J., Asbridge, J.R., Sydoriak, S.J., Solar wind proton properties: Vela 3 observations from July 1965 to June 1967 (1970) Journal of Geophysical Research, 75, p. 4643 | ||
| 504 | |a Mariani, F., Neubauer, F.M., (1990) Physics of the Inner Heliosphere, p. 183. , R., Schwenn, E., Marsch, Springer-Verlag, Berlin | ||
| 504 | |a Marsch, E., Richter, A.K., (1984) J. Geophys. Res., 89, p. 6599 | ||
| 504 | |a Marsch, E., Richter, A.K., (1984) J. Geophys. Res., 89, p. 5386 | ||
| 504 | |a Modisette, J.L., Magnetic Energy Flow in the Solar Wind (1972) The Astrophysical Journal, 174, p. 151 | ||
| 504 | |a Parker, E.N., Dynamics of the Interplanetary Gas and Magnetic Fields. (1958) The Astrophysical Journal, 128, p. 664 | ||
| 504 | |a Pizzo, V., Schwenn, R., Marsch, E., Rosenbauer, H., Muhlhäuser, K.H., Neubauer, F.M., Determination of the solar wind angular momentum flux from the HELIOS data - an observational test of the Weber and Davis theory (1983) The Astrophysical Journal, 271, p. 335 | ||
| 504 | |a Schwenn, R., (1990) Physics of the Inner Heliosphere 1, p. 99. , R., Schwenn, E., Marsch, Springer-Verlag, Berlin | ||
| 504 | |a Weber, E.J., (1970) Solar Phys., 13, p. 240 | ||
| 504 | |a Weber, E.J., Davis, L., The Angular Momentum of the Solar Wind (1967) The Astrophysical Journal, 148, p. 217 | ||
| 504 | |a Weber, E.J., Davis, L., The effect of viscosity and anisotropy in the pressure on the azimuthal motion of the solar wind (1970) Journal of Geophysical Research, 75, p. 2419 | ||
| 504 | |a Whang, Y.C., Conversion of Magnetic-Field Energy Into Kinetic Energy in the Solar Wind (1971) The Astrophysical Journal, 169, p. 369 | ||
| 520 | 3 | |a Solutions already found by one of the authors with a two-region model of the solar coronal expansion are used to analyze the transport of angular momentum and energy by the interplanetary magnetic field. In agreement with observations, it is predicted that the interplanetary magnetic field plays an insignificant role for the flux of energy, but carries a large amount of angular momentum. The appropriate description might be related to the replacement of classical transport coefficients by a collisionless heat flux equation in the outer region of the model. The Sun's loss of angular momentum may affect the strength of the solar rotation in the long term. © 1995 Kluwer Academic Publishers. |l eng | |
| 593 | |a Departamento de Física, Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires, Argentina | ||
| 700 | 1 | |a de la Torre, A. | |
| 773 | 0 | |d Kluwer Academic Publishers, 1995 |g v. 157 |h pp. 367-373 |k n. 1-2 |p Sol Phys |x 00380938 |w (AR-BaUEN)CENRE-2238 |t Solar Physics | |
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| 856 | 4 | 0 | |u https://doi.org/10.1007/BF00680627 |y DOI |
| 856 | 4 | 0 | |u https://hdl.handle.net/20.500.12110/paper_00380938_v157_n1-2_p367_Alexander |y Handle |
| 856 | 4 | 0 | |u https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00380938_v157_n1-2_p367_Alexander |y Registro en la Biblioteca Digital |
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