Showing 1–20 of 23 results
/ Date/ Name
Nov 10, 2010Ultraviolet Coronagraph Spectroscopy: A Key Capability for Understanding the Physics of Solar Wind AccelerationAug 1, 1995Hydrodynamical Simulations of Corotating Interaction Regions and Discrete Absorption Components in Rotating O-Star WindsNov 7, 2012X-Ray Determination of the Variable Rate of Mass Accretion onto TW HydraeApr 18, 2020Solar physics in the 2020s: DKIST, parker solar probe, and solar orbiter as a multi-messenger constellationFeb 14, 2007The Structured Chromosphere and Wind of TW HyaFeb 28, 2012TW Hya: Spectral Variability, X-Rays, and Accretion DiagnosticsJun 25, 2013The Spatial and Temporal Dependence of Coronal Heating by Alfven Wave TurbulenceDec 7, 2014The Role of Turbulence in Coronal Heating and Solar Wind ExpansionMay 7, 2014The Solar Corona as probed by Comet Lovejoy (C/2011 W3)Oct 22, 2014Prevalence of Small-scale Jets from the Networks of the Solar Transition Region and ChromosphereMay 2, 2011Heating of the Solar Chromosphere and Corona by Alfven Wave TurbulenceFeb 13, 2008Hyperdiffusion as a Mechanism for Solar Coronal HeatingJan 5, 2010A Deep Chandra X-ray Spectrum of the Accreting Young Star TW HydraeMay 12, 2014Structure and Dynamics of the Accretion Process and Wind in TW HyaApr 19, 2011The Coronal Physics Investigator (CPI) Experiment for ISS: A New Vision for Understanding Solar Wind AccelerationSep 22, 2008Plasmoids in Reconnecting Current Sheets: Solar and Terrestrial Contexts ComparedOct 26, 2004On the Generation, Propagation, and Reflection of Alfven Waves from the Solar Photosphere to the Distant HeliosphereSep 14, 2023Estimates of Proton and Electron Heating Rates Extended to the Near-Sun EnvironmentJul 23, 2009Electron and proton heating by solar wind turbulenceJan 15, 2010Tangled Magnetic Fields in Solar Prominences