Physics of the Solar Corona and Transition Region

Three-Dimensional Separator Reconnection - How Does It Occur?.- The Structure of Force-Free Magnetic Fields.- Models of Dynamic Coronal Loops.- Cross-Sectional Properties of Coronal Loops.- Width Variations along Coronal Loops Observed by TRACE.- How Accurately Can We Determine the Coronal Heating Mechanism in the Large-Scale Solar Corona?.- SERTS-97 Measurements of Relative Wavelength Shifts in Coronal Emission Lines across a Solar Active Region.- Modeling Coronal Loop Abundances: Effects of Parameter Variations on Observables.- Waves and Oscillations in the Corona.- Can Gravitational Effects Damp Alfvén Waves?.- Observations of the 24 September 1997 Coronal Flare Waves.- Structure of a Large Low-Latitude Coronal Hole.- Electro-Mechanical Coupling between the Photosphere and Transition Region.- The Magnetic Connectivity of Moss Regions.- Magnetic Activity Associated with Radio Noise Storms.- A Kinetic Model of Coronal Heating and Acceleration by Ion-Cyclotron Waves; Preliminary Results.- SECIS: The Solar Eclipse Coronal Eclipse Imaging System.- The SOHO-Stellar Connection.- New Boundary Integral Equation Representation for Finite Energy Force-Free Magnetic Fields in Open Space above the Sun.- Synoptic Maps of Solar Wind; Comparison of IPS Data and the NOAA/SEC Version of the Wang and Sheeley Model.- Topology of Magnetic Field and Coronal Hearing in Solar Active Regions. II. The Role of Quasi-Separatrix Layers.- Recent Theoretical Results on Coronal Heating.- MACS for Global Measurement of the Solar Wind Velocity and the Thermal Electton Temperature during the Total Solar Eclipse on 11 August 1999.- Multi-Wavelength Observations of the 1998 September 27 Flare Spray.