Increases in the area of coronal holes related to interplanetary shocks
Contenido principal del artículo
Resumen
El rastreo de perturbaciones del viento solar por medio del centelleo interplanetario (IPS) de fuentes estelares de radio mostró que las perturbaciones interplanetarias mas importantes se originan en regiones solares que contienen hoyos coronales. A raíz de esto se sugirió que los choques se originan en hoyos coronales cambiantes que repentinamente emiten viento solar más rápido. En este trabajo presentamos dos casos particulares de observaciones solares e interplanetarias relacionadas con comienzos repentinos de tormentas geomagneticas (SC) en los cuales se muestra que el choque interplantetario está relacionado con un aumento en el área de un hoyo coronal. Los eventos considerados corresponden al 6 de junio de 1979 y al 1º. de octubre de 1991. Se describe un escenario solar para la ocurrencia de estos eventos y se presenta un mecanismo para la formación del choque.
Publication Facts
Reviewer profiles N/D
Author statements
- Editor & editorial board
- profiles
- Academic society
- Geofísica Internacional
Para obtener más información sobre un dato, haga clic
PF is maintained by the Public Knowledge Project
Detalles del artículo
Esta obra está bajo una licencia internacional Creative Commons Atribución-NoComercial-CompartirIgual 4.0.
Citas
BRAVO, S., B. MENDOZA and R. PEREZ-ENRIQUEZ, 1991a. Coronal holes as sources of large-scale solar wind disturbances and geomagnetic perturbations. J. Geophys. Res. 96, 5387-5396. DOI: https://doi.org/10.1029/90JA02562
BRAVO, S., B. MENDOZA and R. PEREZ-ENRIQUEZ, 1991 b. Geomagnetic storm sudden commencements and their possible sources at the Sun. Geofísica Internacional, 30, 23-30. DOI: https://doi.org/10.22201/igeof.00167169p.1991.30.1.946
BRAVO, S., 1991. Coronal holes and solar-terrestrial relationships. Geofísica Internacional, 30, 269-272. DOI: https://doi.org/10.22201/igeof.00167169p.1991.30.4.1266
BRAVO, S. and R. PEREZ-ENRIQUEZ, 1993. Coronal mass ejections associated with interplanetary shocks and their relation to coronal holes. Rev. Mexicana Astron. Astrophys. (in press).
DRYER, M., S. T. WU and S. M. HAN, 1980. Two-dimensional time-dependent MHD simulation of the disturbed solar wind due to representative flare-generated and coronal-hole generated disturbances. Geofísica Internacional, 19, 1-15. DOI: https://doi.org/10.22201/igeof.00167169p.1980.19.1.819
DURNEY, B. R. and G. W. PNEUMAN, 1975. Solar-Interplanetary Modeling: 3-D solar wind solutions in prescribed non-radial magnetic field geometries. Solar Phys. 40, 461-485. DOI: https://doi.org/10.1007/BF00162392
HEWISH, A. and S. BRAVO, 1986. The sources of large scale heliospheric disturbances. Solar Phys. 106, 185. DOI: https://doi.org/10.1007/BF00161362
KAHLER, S. W., R. L. MOORE, S. R. KANE and H. ZIRIN, 1988. Filament eruptions and the impulsive phase of solar flares. Astrophys. J. 328, 824-829. DOI: https://doi.org/10.1086/166340
KAHLER, S. W., 1992. Solar flares and coronal mass ejections. Ann. Rev. Astron. Astrophys., 30, 113-141. DOI: https://doi.org/10.1146/annurev.aa.30.090192.000553
KAIGORODOV, A. P. and V. G. FAINSHTEIN, 1991. Diurnal variation of open magnetic tubes from coronal holes and the neutral line on the source surface and related events in the solar wind. Adv. Space Res. 11, #1, 51-54. DOI: https://doi.org/10.1016/0273-1177(91)90089-3
KING, J., 1983. Interplanetary Medium Data Book, Supplement 2, NSSDC/83-01.
LEVINE, R. C., M. D. ALTSCHULER and J. W. HARVEY, 1977. Solar sources of the interplanetary magnetic field and solar wind. J. Geophys. Res. 82, 1061-1065. DOI: https://doi.org/10.1029/JA082i007p01061
PNEUMAN, G. W., 1973. The solar wind and the temperature-density structure of the solar corona. Solar Phys. 28, 247-262. DOI: https://doi.org/10.1007/BF00152928
SHEELEY, Jr. N. R., R. A. HOWARD, M. J. KOOMEN, D. J. MICHELS, R. SCHWENN, K. H. MÜHLHAÜSER and H. ROSENBAUER, 1985. Coronal mass ejections and interplanetary shocks, J. Geophys. Res. 90, 163-175. DOI: https://doi.org/10.1029/JA090iA01p00163
ST. CYR, O. C. and D. F. WEBB, 1991. Activity associated with coronal mass ejections at solar minimum: SMM observations from 1984-1986. Solar Phys., 136, 379-394. DOI: https://doi.org/10.1007/BF00146543
VAN NESS, P., E. C. ROELOF, R. REINHARD, T. R. SANDERSON and K. P. WENZEL, 1985. A major shock-associated energetic storm particle event where in the shock plays a minor role. J. Geophys. Res. 90, 3981-3994. DOI: https://doi.org/10.1029/JA090iA05p03981
WANG, Y. M. and N. R. SHEELEY, Jr., 1990. Solar wind speed and coronal fluxe-tube expansion. Astrophys. J., 355, 726-732. DOI: https://doi.org/10.1086/168805
WANG, Y. M., N. R. SHEELEY, Jr. and A. G. NASH, 1990. Latitudinal distribution of solar wind speed from magnetic observations of the Sun. Nature, 347, 439-444. DOI: https://doi.org/10.1038/347439a0
WANG, Y. M. and N. R. SHEELEY, Jr., 1991. Why fast solar wind originates from slowly expanding coronal flux tubes. Astrophys. J., 372, L45-L48. DOI: https://doi.org/10.1086/186020
WATANABE, T., M. KOJIMA, M. OHYAMA, S. TSUNETA, L. W. ACTON, K. L. HARVEY, J. A. JOSELYN and J. A. KLIMCHUK, 1993. Coronal and interplanetary consequences of a solar-filament disappearance observed with YOHKOH SXT on 28 September 1991. In: Proceedings of the 1992 STEP Symposium, in press.