Showing 21–40 of 43 results
/ Date/ Name
Feb 13, 2008Hyperdiffusion as a Mechanism for Solar Coronal HeatingJan 15, 2010Tangled Magnetic Fields in Solar ProminencesNov 1, 2008Vector Magnetic Fields and Electric Currents from the Imaging Vector MagnetographNov 16, 2012Solar Magnetic Carpet II: Coronal Interactions of Small-Scale Magnetic FieldsJun 10, 2005Slingshot prominences above stellar X-ray coronaeMay 8, 2003Alfvenic Turbulence in the Extended Solar Corona: Kinetic Effects and Proton HeatingAug 15, 2018The Minimum Energy Principle Applied to Parker's Coronal Braiding and Nanoflaring ScenarioMar 14, 2013Observations and modeling of the emerging EUV loops in the quiet Sun as seen with the Solar Dynamics ObservatoryApr 19, 2011The Coronal Physics Investigator (CPI) Experiment for ISS: A New Vision for Understanding Solar Wind AccelerationJul 22, 2002The coronal topology of the rapidly rotating K0 dwarf, AB Doradus I. Using surface magnetic field maps to model the structure of the stellar coronaJul 22, 2007Modelling the Global Solar Corona: Filament Chirality Observations and Surface SimulationsOct 26, 2004On the Generation, Propagation, and Reflection of Alfven Waves from the Solar Photosphere to the Distant HeliosphereDec 17, 2009Comparison of a Global Magnetic Evolution Model with Observations of Coronal Mass EjectionsMar 13, 2007Self-consistent Coronal Heating and Solar Wind Acceleration from Anisotropic Magnetohydrodynamic TurbulenceMar 9, 2004Using Chandra/LETG spectra to probe stellar coronaeMay 21, 2012Proton, Electron, and Ion Heating in the Fast Solar Wind from Nonlinear Coupling Between Alfvenic and Fast-Mode TurbulenceMar 3, 2013Connecting the Sun's High-Resolution Magnetic Carpet to the Turbulent HeliosphereOct 29, 2003The Effect of Proton Temperature Anisotropy on the Solar Minimum Corona and WindAug 4, 2011Solar Magnetic Carpet I: Simulation of Synthetic MagnetogramsDec 8, 2016Direct and Inverse Cascades in the Acceleration Region of the Fast Solar Wind