Large-scale structures and multiple neutral lines associated with coronal mass ejections

Journal of Geophysical Research: Space Physics

Volumn 102, Issue A11, 1997, Pages 24161-24174

  Webb, D F ^a,b   Kahler, S W ^b   McIntosh, P S ^c,e   Klimchuck, J A ^d  

^a BOSTON COLLEGE   (United States)

^b AIR FORCE RESEARCH LABORATORY   (United States)

^c Open Mind Technologies USA Inc   (United States)

^d NAVAL RESEARCH LABORATORY   (United States)

^e Code 7675 JAK ^*  (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 37149034098     PISSN: 01480227     EISSN: None     Source Type: Journal    
DOI: 10.1029/97JA01867     Document Type: Article

References (17)

1. Alexander, D., G.L. Slater, H. S. Hudson, A. H. McAllister, and K. L. Harvey, The large-scale coronal eruptive event of April 14 1994, in Solar Dynamic Phenomena and Solar Wind Consequences, ESA Spec. Publ.-373, p. 187, Eur. Space Agency, ESTEC, Noordwijk, The Netherlands, 1994.
2. Aly, J.J., On some properties of force-free magnetic fields in infinite regions of space, Astrophys. J., 283, 349, 1984.
3. Aly, J.J., How much energy can be stored in a three-dimensional,force-free magnetic field?, Astrophys. J., 375, L61, 1991.
4. Biskamp, D., and H. Welter, Magnetic arcade evolution and instability, Sol Phys., 120, 49, 1989.
5. Cane, H.V., N.R. Sheeley Jr., and H.A. Howard, Energetic interplanetary shocks, radio emission and coronal mass ejections, J. Geophys. Res., 92, 9869, 1987.
6. Chase, R.C., A.S. Krieger, Z. Svestka, and G.S. Vaiana, Skylab observations of X-ray loops connecting separate active regions, Space Res. XVI, 917, 1976.
7. Cliver, E.W., O.C. St. Cyr, H.A. Howard, and P.S. McIntosh, Rotation-averaged rates of coronal mass ejections and dynamics of polar crown filaments, in Solar Coronal Structures; Proceedings of IAU Colloquium 144, edited by V. Rusin et al., p. 83, VEDA, Tatranska Lomnica, Slovak Republic, 1994.
8. Crooker, N.U., G.L. Siscoe, S. Shodhan, P.F. Webb, J.T. Gosling, and E.J. Smith, Multiple heliospheric current sheets and coronal streamer belt dynamics, J. Geophys. Res., 98, 9371, 1993.
9. Eddy, J.A., Observation of a possible neutral sheet in the corona, Sol. Phys., 30, 385, 1973.
10. Feynman, J., and S.F. Martin, The initiation of coronal mass ejections by newly emerging magnetic flux, J. Geophys. Res., 100, 3355, 1995.
11. Forbes, T.G., Magnetic reconnection in solar flares, Geophys. Astrophys. Fluid Dyn., 62, 15, 1991.
12. Forbes, T.G., J.M. Malherbe, and E.R. Priest, The formation of flare loops by magnetic reconnection and chromospheric ablation, Sol. Phys., 120, 285, 1989.
13. Gosling, J.T., The solar flare myth, J. Geophys. Ret., 98, 18,937, 1993.
14. Hansen, S.F., and R.T. Hansen, Differential rotation and reconnection as basic causes of some coronal reorientations, Sol. Phys., 44, 503, 1975.
15. Hansen, S.F., and R.T. Hansen, Reorientation of global coronal magnetic fields due to differential rotation, Sol. Phys., 51, 169, 1977.
16. Harrison, R. A., and G. M. Simnett, Do all flares occur within a hierarchy of magnetic loops?, Adv. Space Res., 4(7), 199, 1984.
17. Wu, S.T., W.P, Guo, and J.F. Wang, Dynamical evolution of a coronal streamer-bubble system, Sol. Phys., 157, 325, 1995.