Session VII

 
• VII: Magnetic Reconnection driven by Surface Alfven Waves in Chromospheric Current Sheets: Lower Coronal Loops Heating
• VII: Theoretical plasma model for intracloud lightning
• VII: Rossby Waves and Vortices in the Solar and Terrestrial Atmospheres
• VII: Increase in sun's magnetic field intensity for Solar Cycles 16 -21
• VII: Total Solar Irradiance and Coronal Index of Solar Activity
• VII: Radio and X-Ray Emissions from Termination Shocks During the November 25, 2000, 09:08 UT Flare
• VII: Evolution of the magnetic field of the active region NOAA 7978 during five disk passages
• VII: White-light eclipse corona and magnetic field connections during the solar cycle
• VII: Magnetic-Flux Emergence into the Solar Corona
• VII: Do Changes in Solar UV Flux Influence a Major Mode of Atmospheric Variability?
• VII: Solar Cycle 23: Variation of the Solar Corona in the Ultraviolet from Solar Minimum to Solar Maximum
• VII: The 88-Year Cycle in the Modulation of the 11-year Solar Cycle Intensity
• VII/III: On relevance of the coronal FeXIV 530.3 nm emission line intensity for studying the cyclic and evolutionary solar processes
• VII/VIII: The Solar Activity Maximum For Cycle 23