Posts about the SHINE workshop.
Authors: Xuanye Ma (ERAU), Katariina Nykyri (ERAU), Simon Wing (JHU/APL), Katherine Holland (ERAU) The solar wind propagates at supersonic speed in the interplanetary medium. Therefore, one wouldView More
Authors: Peter Levens (Cornell University, Stanford University), Aimee A. Norton (HEPL Solar Physics, Stanford University), Kalman J. Knizhnik (Naval Research Laboratory), Mark G. Linton (NavalView More
Authors: Omar Bahri (Utah State University), Pouya Hosseinzadeh (Utah State University), Soukaina Filali Boubrahimi (Utah State University), and Shah Muhammad Hamdi (New Mexico State University)View More
Authors: Collin Brown (University of Iowa), James Juno (Princeton Plasma Physics Laboratory), Greg Howes (University of Iowa), Colby Haggerty (University of Hawaii), Sage Constantinou (UniversityView More
Authors: Thomas Woolley (Imperial College London), Chadi Salem (University of California, Berkeley), Lorenzo Matteini (Imperial College London) Despite being measured over 40 years ago, theView More
Authors: Ronald M. Caplan (Predictive Science Inc.), Tibor Torok (Predictive Science Inc.), Cooper Downs (Predictive Science Inc.), Andres Reyes (Predictive Science Inc.), Viacheslav Titov (PredictiveView More
Authors: Yi Qi (Laboratory for Atmospheric and Space Physics, University of Colorado Boulder, Boulder, CO, USA), T. C. Li (Department of Physics and Astronomy, DartmouthView More
Authors: Rachael Filwett (University of Iowa), Joe Fennell (Aerospace Corporation), Bern Blake (Aerospace Corporation), Allison Jaynes (University of Iowa), Drew Turner (APL), Robert Allen (APL)View More
Authors: C. Kay (NASA GSFC/CUA), T. Nieves-Chinchilla (NASA GSFC), S. J. Hofmeister (Leibniz Institute for Astrophysics), E. Palmerio (Predictive Science) Coronal mass ejections (CMEs) causeView More
Authors: Shanti Thagunna (UAH), Dr. Gary Zank (UAH), Dr. Vladimir Kolobov (UAH) When the mean free path of electrons in plasma is comparable to theView More
Authors: Maria D. Kazachenko (CU Boulder / NSO) What is the difference between confined and eruptive flares in terms of their physical properties at theView More
Authors: Daniel da Silva (NASA/GSFC, UMBC), Nick Arge (NASA/GSFC), Shaela Jones (NASA/GSFC, Catholic University), Samantha Wallace (NASA/GSFC) The origin point on the sun corresponding toView More
Authors: Rebecca Harvey (Department of Space Science, The University of Alabama in Huntsville), Qiang Hu (Department of Space Science, The University of Alabama in Huntsville;View More
Authors: Gregory G. Howes (U Iowa), James Juno (PPPL), Collin R. Brown (U Iowa), Colby C. Haggerty (U Hawaii), Jason M. TenBarge (Princeton U), DamianoView More
Authors: Benjamin Berkey (NCAR/HAO), Joan Burkepile (NCAR/HAO), Marc Cotter (NCAR/HAO), Michael Galloy (NCAR/HAO), Sarah Gibson (NCAR/HAO), Don Kolinski (NCAR/HAO), Enrico Landi (University of Michigan), LisaView More
Authors: Mihailo M. Martinovic (University of Arizona), Kristopher G. Klein (University of Arizona), Tereza Durovcova (Charles University, Prague), Benjamin L. Alterman (Southwest Research Institute) InstabilitiesView More
Authors: Nathaniel H. Mathews (NASA GSFC), Barbara J. Thompson (NASA GSFC) Predicting the current or future state of the coronal magnetic field requires high-resolution modelsView More
Authors: K.G. Klein, H. Spence, & the HelioSwarm Science and Engineering Teams Turbulence is multiscale disorder. It arises in a variety of astrophysical and heliosphericView More
Authors: A. R. Poppe and C. O. Lee The collisional grinding of interplanetary meteoroids should continually produce grains over a wide range of sizes, includingView More
Authors: Niranjana Shankarappa (University of Arizona), Kristopher Klein (University of Arizona) The heating of protons and electrons as the result of the dissipation of turbulenceView More
Authors: Justyna Sokol (SwRI) Solar wind dynamic pressure varies with the solar cycle as measured in the ecliptic plane. The in-ecliptic solar wind speed andView More
Authors: Daniel B. Reisenfeld (Los Alamos National Laboratory), Maciej Bzowski (Space Research Center, Warsaw, Poland), Herbert O. Funsten (Los Alamos National Laboratory), Jacob Heerikhuisen (UniversityView More
Authors: Ratan Kumar Bera (Center for Space Plasma and Aeronomic Research, University of Alabama in Huntsville), Nikolai V Pogorelov (University of Alabama in Huntsville), FedericoView More
Authors: B. J. Lynch (SSL/UCB), N. M. Viall (GSFC/NASA), A. K. Higginson (GSFC/NASA), L. Zhao (CLaSP/UM), S. T. Lepri (CLaSP/UM), X. Sun (IfA/UH) Connecting theView More
Authors: Shea A. Hess Webber (Stanford), Lisa Upton (Southwest Research Institute), Todd Hoeksema (Stanford), Dave Lauben (Stanford), Rock Bush (Stanford) The National Research Council publishedView More
Authors: R. A. Leske(1), A. C. Cummings(1), R. A. Mewaldt(1), E. C. Stone(1), C. M. S. Cohen(1), M. E. Wiedenbeck(2) (1)California Institute of Technology, Pasadena,View More
Authors: J. A. Gilbert (Univ of Michigan), S. T. Lepri (Univ of Michigan), E. Fischer (Univ of Michigan), J. M. Raines (Univ of Michigan), G.View More
Authors: Keiji Hayashi (George Mason University), Chin-Chun Wu (Naval Research Laboratory), Kan Liou (John Hopkins University) The global coronal magnetic field is one of theView More
Authors: Don Kolinski (High Altitude Observatory, National Center for Atmospheric Research), Craig DeForest (Southwest Research Institute), Sarah Gibson (High Altitude Observatory, National Center for AtmosphericView More
Authors: Don Kolinski (High Altitude Observatory, National Center for Atmospheric Research), Robert Allen (Applied Physics Laboratory, Johns Hopkins University), Giuliana de Toma (High Altitude Observatory,View More
Authors: Nishu Karna(CfA), Tatiana Niembro(CfA) Coronal holes are the source of the fast solar wind, and thus play a crucial role in heliophysics as oneView More
Authors: Andrew Alt (Princeton University), Hantao Ji (Princeton University), Jongsoo Yoo (Princeton Plasma Physics Laboratory), Sayak Bose (Princeton Plasma Physics Laboratory), Aaron Goodman (Princeton University),View More
Authors: Michael Hahn (Columbia University), Xiangrong Fu (New Mexico Consortium), Daniel Wolf Savin (Columbia University) We have found evidence for the parametric decay instability (PDI)View More
Authors: Xiaoyan Xie (Harvard-Smithsonian Center for Astrophysics), Katharine Reeves (Harvard-Smithsonian Center for Astrophysics) We deliberately select three flares to investigate heating effects of SADs onView More
Authors: Kathy Reeves (Harvard-Smithsonian Center for Astrophysics) A wide variety of modeling techniques have been used simulate solar eruptions as a means of relating theView More
Authors: Don Schmit (CIRES/CU), Adrian Daw (GSFC/NASA), Jeffrey W. Brosius (Catholic University) , Enrico Landi (University of Michigan), Doug Rabin (GSFC/NASA) The Extreme Ultraviolet NormalView More
Authors: H. Che (UAH), G. P. Zank (UAH), A. O. Benz (FHNW & ETH), B. Tang (UAH) and C. Crawford Observationally, electron beams with power-lawView More
Authors: Heinemann S.G (Max Planck Institute for Solar System Research, 37077 Göttingen, Germany), Yang, D. (Max Planck Institute for Solar System Research, 37077 Göttingen, Germany)View More
Authors: Yeimy Rivera (CfA|Harvard & Smithsonian), John C. Raymond (CfA|Harvard & Smithsonian), Enrico Landi (UMich), Susan T. Lepri (UMich), Ben Alterman (UMich), Kathy Reeves (CfA|HarvardView More
Authors: Valeriy Tenishev (Univeristy of Michigan) Understanding the radiation environment due to solar energetic particles in the heliosphere and the Earth’s magnetosphere is a challengingView More