Correlation between the near-Earth solar wind parameters and the source surface magnetic field

Geomagnetism and Aeronomy

Volumn 46, Issue 4, 2006, Pages 430-437

  Belov, A V ^a   Obridko, V N ^a   Shelting, B D ^a  

^a PUSHKOV INSTITUTE OF TERRESTRIAL MAGNETISM   (Russian Federation)

Author keywords

[No Author keywords available]

Indexed keywords

GEOMAGNETIC FIELD; NUMERICAL MODEL; SOLAR WIND; STATISTICAL ANALYSIS;

EID: 33750914651     PISSN: 00167932     EISSN: 1555645X     Source Type: Journal    
DOI: 10.1134/S0016793206040049     Document Type: Article

References (11)

1. S. I. Akasofu, "The Solar Wind-Magnetosphere Energy Coupling and Magnetosphere Disturbances" Planet. Space Sci. 28, 495-509 (1980).
2. A. V. Belov, S. P. Gaidash, Kh. D. Kanonidi, et al., Operative Center of the Geophysical Prognosis (IZMIRAN, 2005), Ann. Geophysical 23 (9), 3163-3170 (2005).
3. J. T. Hoeksema and P. H. Scherrer, The Solar Magnetic Field (Rep. UAG-94, NOAA, Boulder, 1986).
4. V. N. Obridko, B. D. Shelting, and A. F. Kharshiladze, "Multiparametric Calculations of the Solar Wind Parameters from Data on the Solar Magnetic Field," Astron. Vestn. 38 (3), 261-272 (2004).
5. V. N. Obridko, B. D. Shelting, and A. F. Kharshiladze, "Near-Earth Magnetic Field Calculations from Data on Solar Magnetic Field," Geomagn. Aeron. 46 (3), 2006.
6. V. N. Obridko, A. F. Kharshiladze, and B. D. Shelting, "On calculating the solar wind parameters from the solar magnetic field data," Astron. Astrophys. Trans. 11, 65-79 (1996)
7. V. N. Oraevsky, Kh. D. Kanonidi, A. V. Belov, and S. P. Gaidash, "Operative Center IZMIRAN on Forecasting of Heliophysical Conditions. Problem of the Forecasting of Extreme Situations and Their Sources," in Proceedings of the Research-Practical Conference on 26-27 June 2001 (Center "Antistikhiya", 2002), pp. 222-229.
8. Y. M. Wang and N. R. Sheeley, "On Potential Field Models of the Solar Corona," Astrophys. J. 392, 310-319 (1992).
9. Y. M. Wang and N. R. Sheeley, "Solar Wind Speed and Coronal Flux Tube Expansion," Astrophys. J. 335, 726-732 (1990).
10. Y. M. Wang and N. R. Sheeley, "Why Fast Solar Wind Originates from Slowly Expanding Coronal Flux Tubes," Astrophys. J. 372, L45-48 (1991).
11. Y. M. Wang, "Energy Coupling between the Solar Wind and the Magnetosphere," Space Sci. Rev. 28, 121 (1981).