The FIP Effect on Individual Charge State Abundances
Authors: D. Carpenter (University of Michigan), L. Zhao (University of Michigan), S. T. Lepri (University of Michigan) In this work, we analyze the individual chargeView More
Authors: D. Carpenter (University of Michigan), L. Zhao (University of Michigan), S. T. Lepri (University of Michigan) In this work, we analyze the individual chargeView More
Authors: Katariina Nykyri (Embry-Riddle Aeronautical University), Xuanye Ma (Embry-Riddle Aeronautical University), Roberto Cuellar Rangel (Embry-Riddle Aeronautical University), Jef Broll (LANL), Joe Borovsky (Space Science Institute),View More
Authors: Aatiya Ali (Georgia State University), Viacheslav Sadykov (Georgia State University), Alexander Kosovichev (New Jersey Institute of Technology) Solar energetic particles (SEPs) and their propagationView More
Authors: Rohit Chhiber (University of Delaware & NASA GSFC), William Matthaeus (University of Delaware), Arcadi Usmanov (University of Delaware & NASA GSFC), Riddhi Bandyopadhyay (PrincetonView More
Authors: Samuel Badman (UC Berkeley/Space Sciences Lab) This scene-setting talk will review current and upcoming models of the coupled coronal and heliospheric system in termsView More
Authors: Young Dae Yoon (Pohang Accelerator Laboratory), Deirdre E. Wendel (NASA GSFC), Gunsu S. Yun (POSTECH) From the Harris equilibrium to the force-free equilibrium, thereView More
Authors: Arturo Tinoco-Arenas (Instituto de Geofísica UNAM) , Primož Kajdič (Instituto de Geofísica UNAM), Luis Preisser (Space Research Institute / Austrian Academy of Science )View More
Authors: Carlos Arturo Perez-Alanis (Universidad Nacional Autónoma de México, UNAM), Miho Janvier (Universit ́e Paris-Saclay, CNRS, Institut d’Astrophysique Spatiale, Orsay, France), Teresa Nieves-Chinchilla (Heliophysics ScienceView More
Authors: Zihao Yang (Peking University; NCAR/HAO), Hui Tian (Peking University), Xianyong Bai (NAOC), Yajie Chen (Peking Univerisity), Yang Guo (Nanjing University), Yingjie Zhu (University ofView More
Authors: Zihao Yang (Peking University; NCAR/HAO), Christian Bethge (USRA), Hui Tian (Peking University), Steven Tomcyzk (NCAR/HAO), Richard Morton (Northumbria University), Giulio Del Zanna (University ofView More
Authors: Ivan Vasko (UC Berkeley), Ajay Lotekar (IRF, Sweden), Tai Phan (UC Berkeley), Kaz Alimov (UC Berkeley), Stuart Bale (UC Berkeley), Forrest Mozer (UC Berkeley),View More
Authors: Satoshi Inoue (Center for Solar-Terrestrial Research, New Jersey Institute of Technology), Keiji Hayashi (George Mason University), Takahiro Miyoshi (Graduate School of Science, Hiroshima UniversityView More
Authors: H. Y. Wei (Dept. of Earth, Planetary and Space Sciences, University of California, Los Angeles, CA, USA), L. K. Jian (NASA Goddard Space FlightView More
Authors: Wenyuan Yu (University of New Hampshire), Nada A. Al-Haddad (University of New Hampshire), Charles J. Farrugia (University of New Hampshire), Noé Lugaz (University ofView More
Authors: Giuliana de Toma (HAO/NCAR) The period of solar minimum and rising phase of solar cycle 25 is examined using HMI magnetic field and sunspotView More
Authors: Piyush Agrawal (Southwest Research Institute), Lisa Upton (Southwest Research Institute) Understanding the motions of solar photospheric magnetic fields is crucial, as they are aView More
Authors: Holly Gilbert (HAO), Steven Tomczyk (HAO), Sarah Gibson (HAO, Enrico Landi (U. of Michigan), Haosheng Lin (U. of Hawaii), Ed DeLuca (Harvard Smithsonian CfA),View More
Authors: Sarah A. Spitzer (University of Michigan), Susan T. Lepri (University of Michigan), Jim M. Raines (University of Michigan), Frederic Allegrini (Southwest Research Institute), ConnorView More
Authors: Philip Quinn (NASA/JSC/SRAG (Leidos)) In human exploration operations, space weather forecasting models are used to help predict the severity of solar particle events. ButView More
Authors: S.D. Bale, T. S. Horbury, L.Matteini, T. Woolley, J. Stawarz, L.D. Woodham Parker Solar Probe’s (PSP’s) 11th encounter in February 2022 has provided aView More
Authors: Opal Issan (University of California, San Diego ), Boris Kramer (University of California, San Diego ) Solar wind conditions are predominantly predicted via three-dimensionalView More
Authors: Donald M. Hassler (SwRI), Tania Varesano (SwRI), Natalia Zambrana Prado (GSFC), Alessandra Giunta (RAL), Joseph Plowman (SwRI) The Spectral Imaging of the Coronal EnvironmentView More
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