Causal relationships between eruptive prominences and coronal mass ejections

Annales Geophysicae

Volumn 26, Issue 10, 2008, Pages 3025-3031

  Filippov, B ^a   Koutchmy, S ^b  

^a PUSHKOV INSTITUTE OF TERRESTRIAL MAGNETISM   (Russian Federation)

^b INSTITUT D'ASTROPHYSIQUE DE PARIS   (France)

Author keywords

[No Author keywords available]

Indexed keywords

CORONA; CORONAL MASS EJECTION; MAGNETIC FIELD;

EID: 54249141495     PISSN: 09927689     EISSN: 14320576     Source Type: Journal    
DOI: 10.5194/angeo-26-3025-2008     Document Type: Article

References (43)

1. Alexander, D., Liu, R., and Gilbert, H.: Hard X-ray production in a failed filament eruption, Astrophys. J., 653, 719-724, 2006.
2. Boulade,~S., Delannée,~C., Koutchmy,~S., Lamy,~P., Llebaria,~A., Howard,~R., Schwenn,~R., and Simnett,~G.: Analysis of a high latitude slow CME with travelling ejecta, The Corona and Solar Wind Near Minimum Activity, edited by: Wilson, A., ESA SP, 404, 217-221, 1997.
3. Chen,~J.: Effects of toroidal forces in current loops embedded in a background plasma, Astrophys. J., 338, 453-470, 1989.
4. Chen, J. and Krall, J.: Acceleration of coronal mass ejections, J. Geophys. Res., 108 (A11), 1410, doi:10.1029/2003JA009849, 2003.
5. Chen, J., Marque, C., Vourlidas, A., Krall, J., and Schick, P. W.: The flux-rope scaling of the acceleration of coronal mass ejections and eruptive prominences, Astrophys. J., 649, 452-463, 2006.
6. Cliver, E. W. and Webb, D. F.: Disappearances of high-latitude filaments as sources of high-latitude CMEs, New Perspectives on Solar Prominences, edited by: Webb, D., Rust, D., and Schmieder, B., ASP Conference Series, ASP, San Francisco, CA, 150, 479-483, 1998.
7. Crifo, F., Picat, J. P., and Cailloux, M.: Coronal transients - loop or bubble, Sol. Phys., 83, 143-152, 1983.
8. Demoulin,~P. and Priest,~E R.: A twisted flux model for solar prominences. II - Formation of a dip in a magnetic structure before the formation of a solar prominence, Astron. Astrophys., 214, 360-368, 1989.
9. Filippov, B. P. and Den, O. G.: Prominence height and vertical gradient in magnetic field, Astron. Lett., 26, 322-327, 2000.
10. Filippov, B. P. and Den, O. G.: A critical height of quiescent prominences before eruption. J. Geophys. Res., 106, 25 177-25 184, 2001.
11. Filippov, B. P., Gopalswamy, N., and Lozhechkin, A. V.: Non-radial motion of eruptive filaments, Sol. Phys., 203, 119-130, 2001.
12. Filippov, B. P., Gopalswamy, N., and Lozhechkin, A. V.: Motion of an eruptive prominence in the solar corona, Astron. Rep., 46, 417-422, 2002.
13. Filippov, B. P. and Koutchmy, S.: About the prominence heating mechanisms during its eruptive phase, Sol. Phys., 208, 283-295, 2002.
14. Foley, C. R., Harra, L. K., Matthews, S. A., Culhane, J. L., and Kitai, R.: Evidence for a flux rope driven EUV wave and CME: comparison with the piston shock model, Astron. Astrophys., 399, 749-754, 2003.
15. Forbes, T. G. and Isenberg, P. A.: A catastrophe mechanism for coronal mass ejections, Astrophys. J., 373, 294-307, 1991.
16. Gibson, S. E. and Low, B. C.: A time-dependent three-dimensional magnetohydrodynamic model of the coronal mass ejection, Astrophys. J., 493, 460-473, 1998.
17. Gilbert, H. R., Holzer, T. E., Burkepile, J. T., and Hunhausen, A. J.: Active and eruptive prominences and their relationship to coronal mass ejections, Astrophys. J., 537, 503-515, 2000.
18. Gopalswamy, N., Shimojo, M., Lu, W., Yashiro, S., Shibasaki, K., and Howard, R. A.: Prominence eruptions and coronal mass ejection: a statistical study using microwave observations, Astrophys. J., 586, 562-578, 2003.
19. House, L. L., Wagner, W. J., Hildner, E., Sawyer, C., and Schmidt, H. U.: Studies of the corona with the Solar Maximum Mission coronagraph/polarimeter, Astrophys. J., 244, L117-L121, 1981.
20. Koutchmy,~S., Baudin,~F., Bocchialini,~K., Daniel,~J.-Y., Delaboudinière,~J.-P., Golub,~L., Lamy,~P., and Adjabshirizadeh,~A.: The 11th August 1999 CME, Astron. Astrophys., 420, 709-718, 2004.
21. Koutchmy, S., Filippov, B., and Lamy, Ph.: Old and new aspects of prominence physics from coronal observations, The Physics of Chromospheric Plasmas,edited by: Heinzel, P., Dorotoviè, I., and Rutten, R. J., ASP Conference Series, ASP, San Francisco, CA, 368, 331-336, 2007.
22. Krall,~J. and Chen,~J.: Density structure of a preeruption coronal flux rope, Astrophys. J., 628, 1046-1055, 2005.
23. Krall,~J. and Sterling, A. C.: Analysis of erupting solar prominences in terms of an underlying flux-rope configuration, Astrophys. J., 663, 1354-1362, 2007.
24. Kuperus,~M. and Raadu,~M A.: The support of prominences formed in neutral sheets, Astron. Astrophys., 31, 189-193, 1974.
25. Lin, J.: CME-flare association deduced from catastrophic model of CMEs, Sol. Phys., 219, 169-196, 2004.
26. Lin, J., Forbes, T. G., Isenberg, P. A., and Demoulin, P.: The effect of curvature on flux-rope models of coronal mass ejections, Astrophys. J., 504, 1006-1019, 1998.
27. Low,~B C. and Hundhausen,~A J.: The velocity field of a coronal mass ejection - The event of 1 September 1980, J. Geophys. Res., 92, 2221-2230, 1987.
28. Marièi\ae,~D., Vr?nak,~B., Stanger,~A L., and Veronig,~A.: Coronal mass ejection of 15 May 2001: I. Evolution of morphological features of the eruption, Sol. Phys., 225, 337-353, 2004.
29. Molodensky, M. M. and Filippov, B. P.: Rapid Motion of Filaments in Solar Active Regions. II, Sov. Astron., 31, 564-568, 1987.
30. Mouradian, Z., Soru-Escaut, I., and Pojoga, S.: On the two classes of filament-prominence disappearance and their relation to coronal mass ejections, Sol. Phys., 158, 269-281, 1995.
31. Mouschovias,~T Ch. and Poland,~A I.: Expansion and broadening of coronal loop transients - A theoretical explanation, Astrophys. J., 220, 675-682, 1978.
32. Munro, R. H., Cosling, J. T., Hildner, E., Mac Queen, R. M., Poland, A. I., and Ross, C. L.: the association of coronal mass ejection transients with other forms of solar activity, Sol. Phys., 61, 201-215, 1979.
33. Sime, D. G., MacQueen, R. M., and Hundhausen, A. J.: Density distribution in looplike coronal transients - A comparison of observations and a theoretical model, J. Geophys. Res., 89, 2113-2121, 1984.
34. Torok,~T. and Kliem,~B.: Confined and ejective eruptions of kink-unstable flux ropes, Astrophys. J., 630, L97-L100, 2005.
35. Van Tend, W. and Kuperus, M.: The development of coronal electric current system in active regions and their relation to filaments and flares, Sol. Phys., 59, 115-127, 1978.
36. Vrsnak,~B.: Eruptive instability of cylindrical prominences, Sol. Phys., 129, 295-312, 1990.
37. Vrsnak,~B., Ruzdjak,~V., Brajsa,~R., and Zloch,~F.: Oscillatory motions in an active prominence, Sol. Phys., 127, 119-126, 1990.
38. Vrsnak, B., Rosa, D., Bozic, H. et al.: Height of tracers and the correction of the measured solar synodic rotation rate: demonstration of the method, Sol. Phys., 185, 207-225, 1999.
39. Webb, D. F., Krieger, A. S., and Rust, D. M.: Coronal X-ray enhancements associated with H-alpha filament disappearances, Sol. Phys., 48, 159-186, 1976.
40. Webb, D. F., Hundhausen, A. J.: Activity associated with the solar origin of coronal mass ejections, Sol. Phys., 108, 383-401, 1987.
41. Westin,~H. and Liszka,~L.: Motion of ascending prominences, Sol. Phys., 11, 409-424, 1970.
42. Yang, G. and Wang, Y.: Statistical Studies of Filament Disappearances and CMEs, Magnetic Activity and Space Environment; edited by: Wang, H. N., Xu, R. L., Proc. COSPAR Colloq., Pergamon, Boston, Ser. 14, 113-116, 2002.
43. Zagnetko, A. M., Filippov, B. P., and Den O. G.: Geometry of solar prominences and magnetic fields in the corona, Astron. Rep., 49, 425-430, 2005.