References

(The references beginning with letter codes, like KUL1, can be found in the description of the different members of the consortium in Section 3.)

1.

R. Keppens and G. Toth: ``Nonlinear dynamics of Kelvin-Helmholtz unstable magnetized jets: Three-dimensional effects'', Phys. Plasmas, 6, 1461-1469 (1999).

2.

R.C. Canfield, H.S. Hudson and D.E. McKenzie: ``Sigmoidal morphology and eruptive solar activity'', Geophys. Res. Lett., 26, 627 (1999).

3.

R.M.E. Illing and A.J. Hundhausen: ``Observation of a coronal transient from 1.2 to 6 solar radii'', J. Geophys. Res., 90, 275-282 (1985).

4.

J. Feynman and S.F. Martin: ``The initiation of coronal mass ejections by newly emerging magnetic flux'', J. Geophys. Res., 100, 3355-3367 (1995).

5.

H.S. Hudson, J.R. Lemen, O.C. St. Cyr, A.C. Sterling, D.F. Webb: ``X ray coronal changes during halo CMEs'', Geophys. Res. Lett., 25, 2481 (1998).

6.

B.J. Thompson, J.B. Gurman, W.M. Neupert, J.S. Newmark, J.-P. Delaboudiniere, O.C. St. Cyr, S. Stezelberger, K.P. Dere, R.A. Howard, D.J. Michels: ``SOHO/EIT Observations of the 1997 April 7 Coronal Transient: Possible Evidence of Coronal Moreton Waves'', Astrophys. J., 517, L151-L154 (1999).

7.

A.J. Hundhausen and T.E. Holzer and B.C. Low: ``Do slow shocks precede some coronal mass ejections?'', J. Geophys. Res., 92 A10, 11,173-11,178 (1987).

8.

L. Burlaga et al.: ``A magnetic cloud containing prominence material: January 1997'', J. Geophys. Res., 103 A1, 277-285 (1998).

9.

J.T. Gosling, W.C. Feldman, D.J. McComas, J.L. Phillips, V.J. Pizzo, and R.I. Forsyth: ``ULYSSES observations of opposed tilts of solar wind corotating interaction regions in the northern and southern solar hemispheres'', GRL, 22, 3333-3336 (1995).

10.

D. Odstrcil and V.J. Pizzo: ``Three-dimensional propagation of coronal mass ejections in a structured solar wind flow, 2, CME launched adjacent to the streamer belt'', J. Geophys. Res., 104, pp. 493 (1999).

11.

D. Odstrcil and V.J. Pizzo: ``Three-dimensional propagation of CMEs in a structured solar wind flow, 1, CME launched within the streamer belt'', J. Geophys. Res., 104, pp. 483 (1999).

12.

D. Odstrcil and V.J. Pizzo: ``Distortion of the interplanetary magnetic field by three-dimensional propagation of coronal mass ejections in a structured solar wind'', J. Geophys. Res., 104, pp. 28225 (1999).

13.

Z. Smith, D. Odstrcil, M. Dryer: ``A 2.5-dimensional MHD parametric study of interplanetary shock interactions with the heliospheric current sheet/heliospheric plasma sheet'', J. Geophys. Res., 103, pp. 20581 (1998).

14.

S.T. Wu, W.P. Guo, D.J. Michels, and L.F. Burlaga: ``MHD description of the dynamical relationships beween a flux rope, streamer, coronal mass ejection, and magnetic cloud: An analysis of the January, 1997 Sun-Earth connection event'', J. Geophys. Res., 104, pp. 14789 (1999).

15.

V.J. Pizzo, D.S. Intriligator, and G.L. Siscoe: ``Radial alignment simulation of solar wind streams observed by Pioneers 10 and 11 in 1974 '', J. Geophys. Res., 100, pp. 12251 (1995).