Initial localization and kinematic characteristics of the structural components of a coronal mass ejection

Journal of Geophysical Research: Space Physics

Volumn 110, Issue A5, 2005, Pages

  Uralov, A M ^a   Grechnev, V V ^a   Hudson, H S ^b  

^a INSTITUTE OF SOLAR TERRESTRIAL PHYSICS   (Russian Federation)

^b UNIVERSITY OF CALIFORNIA   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 33747121538     PISSN: None     EISSN: 21699402     Source Type: Journal    
DOI: 10.1029/2004JA010951     Document Type: Article

References (18)

1. Barenblatt, G. I. (1978), Similarity, Self-Similarity, and Intermediate Asymptotics (in Russian), 207 pp., Gidrometeoizdat, Leningrad.
2. Chertok, I. M., V. V. Grechnev, H. S. Hudson, and N. V. Nitta (2004), Homologous large-scale activity in solar eruptive events of 24-26 November 2000, J. Geophys. Res., 109, A02112, doi:10.1029/2003JA010182.
3. Cremades, H., and V. Bothmer (2004), On the three-dimensional configuration of coronal mass ejections, Astron. Astrophys., 422, 307.
4. Dere, K. P., et al. (1997), EIT and LASCO Observations of the Initiation of a Coronal Mass Ejection, Solar Phys., 175(2), 601-612.
5. Gallagher, P. T., G. R. Lawrence, and B. R. Dennis (2003), Rapid acceleration of a coronal mass ejection in the low corona and implications for propagation, Astrophys. J., 588(1), L53-L56.
6. Grechnev, V. V., et al. (2003), The Siberian Solar Radio Telescope: the current state of the instrument, observations, and data, Solar Phys., 216(1), 239-272.
7. Harrison, R. A., P. Bryans, G. M. Simnett, and M. Lyons (2003), Coronal dimming and the coronal mass ejection onset, Astron. Astrophys., 400, 1071-1083.
8. Hudson, H. S., L. W. Acton, K. L. Harvey, and D. E. McKenzie (1999), A stable filament cavity with a hot core, Astrophys. J., 513, L83-L86.
9. Kano, R. (1994), The time evolution of X-ray structure during filament eruption, in X-ray Solar Physics from Yohkoh, edited by Y. Uchida et al., p. 273, Universal Acad. Press, Tokyo.
10. Khan, J. I., and H. S. Hudson (2000), Homologous sudden disappearances of transequatorial interconnecting loops in the solar corona, Geophys. Res. Lett, 27, 1083.
11. Low, B. C. (1982), Self-similar magnetohydrodynamics. I - The gamma = 4/3 polytrope and the coronal transient, Astrophys. J., 254, 796-805.
12. Martin, S. F. (1998), Conditions for the formation and maintenance of filaments (invited review), Solar Phys., 182, 107-137.
13. Neupert, W. M. (2002), Acceleration of coronal mass ejections in the low corona and association with surface activity, 200th AAS Meeting, Bull. Am. Astron. Soc., 34, 693.
14. Sedov, L. I. (1981), Similarity Methods and Dimensional Analysis in Mechanics (in Russian), 9th ed., 448 pp., Nauka, Moscow.
15. Smolkov, G. I., A. A. Pistolkors, T. A. Treskov, B. B. Krissinel, and V. A. Putilov (1986), The Siberian solar radio-telescope - Parameters and principle of operation, objectives and results of first observations of spatio-temporal properties of development of active regions and flares, Astrophys. Space Sci., 119(1), 1-4.
16. Uralov, A. M., S. V. Lesovoi, V. G. Zandanov, and V. V. Grechnev (2002), Dual-filament initiation of a Coronal Mass Ejection: Observations and model, Solar Phys., 205(1), 69-90.
17. Wang, H., Y. Yan, T. Sakurai, and M. Zhang (2000), Topology of magnetic field and coronal heating in solar active regions - II. The role of quasi-separatrix layers, Solar Phys., 797(2), 263-273.
18. Zel'dovich, Y. B., and Y. P. Raizer (1966), Physics of Shock Waves and High-Temperature Hydrodynamic Phenomena (in Russian), 2nd ed., 686 pp., Nauka, Moscow.