Content-Length: 223379 | pFad | https://helioshine.org/tag/shine2024-session-17/
Associated with SHINE 2024 Session 17
Authors: Andrew McCubbin (JHU APL), Carlos Braga (JHU APL), Evangelia Samara (NASA GSFC), Viacheslav Merkin (JHU APL) With the rise in solar activity, the ParkerView More
Authors: Gabor Toth (University of Michigan), Bart van der Holst (University of Michigan), Xiantong Wang (University of Michigan) Extended magnetohydrodynamic (XMHD) involves extra variables and/orView More
Authors: Federico Fraternale (Center for Space Plasma and Aeronomic Research, The University of Alabama in Huntville) The interaction of the solar wind with the localView More
Authors: Bin Chen (NJIT), Dale Gary (NJIT), Gelu Nita (NJIT), Sijie Yu (NJIT), Pascal Saint-Hilaire (UC Berkeley), Gregg Hallinan (Caltech), and the EOVSA and OVRO-LWAView More
Authors: Jia Huang (SSL/UCB), the SWEAP and FIELDS teams The slow solar wind is typically characterized as having low Alfvénicity. However, Parker Solar Probe (PSP)View More
Authors: Tong Shi (SETI Institute), Ward Manchester IV (University of Michigan), Enrico Landi (University of Michigan), Bart van der Holst (University of Michigan), Judit SzenteView More
Authors: Rohit Chhiber (NASA GSFC & U Delaware), Arcadi Usmanov (NASA GSFC & U Delaware), William Matthaeus (U Delaware), Melvyn Goldstein (SSI), and Others TheView More
Authors: Guanglu Shi (Purple Mountain Observatory), Li Feng (Purple Mountain Observatory), Beili Ying (Purple Mountain Observatory), Shuting Li (Purple Mountain Observatory), Weiqun Gan (Purple MountainView More
Authors: Rohit Chhiber (NASA GSFC & U Delaware) (Draft:) Global inner-heliospheric magnetohydrodynamic (MHD) models aim to represent large-scale properties of the solar wind from theView More
Authors: Y. J. Rivera (Center for Astrophysics | Harvard & Smithsonian), J. Samra (Center for Astrophysics | Harvard & Smithsonian), S. T. Badman (Center forView More
Authors: Jamie M. Jasinski (NASA Jet Propulsion Laboratory), Corey J. Cochrane (NASA Jet Propulsion Laboratory), Xianzhe Jia (University of Michigan), William R. Dunn (UCL), EliasView More
Authors: Caroline L. Evans (University of Colorado Boulder), Cooper Downs (Predictive Science, Inc.), Don Schmit (Cooperative Institute for Research in Environmental Sciences), James Crowley (UniversityView More
Authors: James Crowley (National Solar Observatory; CU Boulder), Cooper Downs (Predictive Science Inc.), Don Schmit (CIRES), Caroline Evans (National Solar Observatory; CU Boulder) Over theView More
Authors: Steven Cranmer (University of Colorado Boulder) Many different physical processes have been suggested to explain the origen of the corona and solar wind. AView More
Authors: Daniel Mendoza (CU Boulder, LASP) Steven Cranmer ( CU Boulder, LASP) There are many methods available for extrapolating the Sun’s magnetic field from theView More
Authors: Yang Liu (Stanford University), J. T. Hoeksema (Stanford University), Luca Bertello (NSO), Gordon Petrie (NSO), Alexei Pevtsov (NSO), Charles Arge (NASA), Sheala Jones (NASA)View More
Fetched URL: https://helioshine.org/tag/shine2024-session-17/
Alternative Proxies: