Physics of the Solar Corona and Transition Region. Questo articolo non è disponibile.Physics of the Solar Corona and Transition Region

staffofKluwerfor theproductionofthetopicalissuesandtheirreprints. Thepapers acceptedforthisTopicalIssueadduptosuchavolumethattheyhaveto be distributedovertwo TopicalIssues of SolarPhysics (December 1999and April 2000),which are reprintedin two bound volumes, of whichthis is the second.

Three-Dimensional Separator Reconnection - How Does It Occur? K. Galsgaard, et al. The Structure of Force-Free Magnetic Fields; E.A. Evangelidis, et al. Models of Dynamic Coronal Loops; G. Peres. Cross-Sectional Properties of Coronal Loops; J.A. Klimchuk. Width Variations along Coronal Loops Observed by TRACE; J.A. Watko, J.A. Klimchuk. How Accurately Can We Determine the Coronal Heating Mechanism in the Large-Scale Solar Corona? D.H. Mackay, et al. SERTS-97 Measurement of Relative Wavelength Shifts in Coronal Emission Lines across a Solar Active Region; J.W. Brosius, et al. Modeling Coronal Loop Abundances: Effects of Parameter Variations on Observables; D.D. Lenz. Waves and Oscillations in the Corona; B. Roberts. Can Gravitational Effects Damp Alfvén Waves? J.F. McKenzie, W.I. Axford. Observations of the 24 September 1997 Coronal Flare Waves; B.J. Thompson, et al. Structure of a Large Low-Latitude Coronal Hole; B.J.J. Bromage, et al. Electro-Mechanical Coupling between the Photosphere and Transition Region; T.D. Tarbell, et al. The Magnetic Connectivity of Moss Regions; X.P. Zhao, et al. Magnetic Activity Associated with Radio Noise Storms; R.D. Bentley, et al. A Kinetic Model of Coronal Heating and Acceleration by Ion-Cyclotron Waves: Preliminary Results; P.A. Isenberg, et al. SECIS: The Solar Eclipse Coronal Eclipse Imaging System; K.J.H. Phillips, et al. The SOHO-Stellar Connection; T.R. Ayres.