Authors: Parisa Mostafavi (Johns Hopkins University Applied Physics Lab), Gary Zank, Matt Hill, Merav Opher, Pontus Brandt, Marc Kornblouth, Ralph McNutt, Dave McComas, and NewView More
Authors: Pertti Makela (CUA), Nat Gopalswamy(NASA/GSFC), Sachiko Akiyama (CUA), Hong Xie (CUA), Seiji Yashiro (CUA) Sustained gamma-ray emission (SGRE) events are solar eruptions that showView More
Authors: M. A. Dayeh (Southwest Research Institute and University of Texas at San Antonio), E. J. Zirnstein (Princeton University), P. Swaczyna (Space Research Centre PAS,View More
Authors: Pierre-Simon Mangeard (University of Delaware, USA), John Clem (University of Delaware, USA), Paul Evenson (University of Delaware, USA), Warit Mitthumsiri (Mahidol University, Thailand), PradiphatView More
Authors: Noé Lugaz (UNH), Camilla Scolini (UNH), Bin Zhuang (UNH), Charles J. Farrugia (UNH), Nada Al-Haddad (UNH), Réka Winslow (UNH), Florian Regnault (UNH), Wenyuan YuView More
Authors: Andrew M. Leisner (George Mason University), Jeremey A. Grajeda (New Mexico State University), C. Nick Arge (NASA/GSFC), Michael Kirk (ASTRA), Laura Boucheron (New MexicoView More
Authors: J. Grant Mitchell (NASA/GSFC), Georgia A. de Nolfo (NASA/GSFC), Jim Ryan (UNH), Alessandro Bruno (NASA/GSFC) Fast neutrons ( > 0.5 MeV) are ubiquitous inView More
Authors: Ioannis Kontogiannis (Leibniz-Institute for Astrophysics Potsdam (AIP), Germany) The emergence of magnetic flux often leads to complex magnetic field configurations, which carry strong electricView More
Authors: Chen Shi (UCLA), Nikos Sioulas (UCLA), Zesen Huang (UCLA), Marco Velli (UCLA), Anna Tenerani (UT Austin) We carry out 3D magnetohydrodynamic (MHD) simulations ofView More
Authors: Ian Berry (Institute for Astronomy, University of Hawai’i’), Xudong Sun (Institute for Astronomy, University of Hawai’i’), Sarah Jaeggli (National Solar Observatory), Wei Liu (LockheedView More
Authors: Ying Wang Eruptive events are the major sources of solar wind and bring magnetic fields and energeticparticles from the solar surface to the nearView More
Authors: Gilchrst, S.A. (Planetary Science Institute), Odgren, M. (Planetary Science Institute, Evergreen High School), Welsch, B.T. (University of Wisconsin-Green Bay) Sigmoids are S-shaped structures seenView More
Authors: Shah Mohammad Bahauddin (University of Colorado Boulder) The high spatial resolution and fast temporal cadence of the current generation of observing instruments, such asView More
Authors: Sumanth Rotti (Georgia State University), Petrus Martens (Georgia State University) Reliable predictions of SEP events are vital to mitigate and avoid space weather hazards,View More
Authors: Cooper Downs (Predictive Science Inc), Jon A. Linker (Predictive Science Inc), Ronald M. Caplan (Predictive Science Inc), and the Solo/PHI team (MPS) The keyView More
Authors: Tarik M. Salman (NASA/GSFC & GMU), Teresa Nieves-Chinchilla (NASA/GSFC), Lan K. Jian (NASA/GSFC), Noé Lugaz (UNH), Fernando Carcaboso (NASA/GSFC) The historic Parker Solar ProbeView More
Authors: Shaheda Begum Shaik (George Mason University), Mark Linton (Naval Research Laboratory), Sarah Gibson (National Center for Atmospheric Research),Phillip Hess (Naval Research Laboratory), Robin ColaninnoView More
Authors: Michael Terres (The University of Alabama in Huntsville), Gang Li (The University of Alabama in Huntsville) The dynamics of the solar wind are thoughtView More
Authors: Syed Raza (UAH), Nikolai Pogorelov (UAH), Talwinder Singh (UAH) In this study, we aim to improve the accuracy of arrival time predictions for MHDView More
Authors: Jiayi Liu (University of Hawaii), Xudong Sun (University of Hawaii), Peter Schuck (NASA Goddard Space Flight Center), Sarah Jaeggli (NSO), Brian Welsch (University ofView More
Authors: Elliot Johnson (University of Delaware) Collisional analysis combines the effects of collisional relaxation and large-scale expansion to determine how solar wind parameters evolve asView More
Authors: Christopher Light (NASA-CCMC), Claudio Corti (NASA-CCMC), M Leila Mays (NASA-CCMC), Beatriz Sanchez-Cano (University of Leicester), David Lario (NASA-GSFC), Alessandro Bruno (NASA-GSFC), Ian Richardson (NASA-GSFC),View More
Authors: S. Roy (Center for Astrophysics | Harvard & Smithsonian), K. Reeves (Center for Astrophysics | Harvard & Smithsonian), C. Moore (Center for Astrophysics |View More
Authors: Jon A. Linker (Predictive Science Inc.), Cooper Downs (Predictive Science Inc.), Ronald M. Caplan (Predictive Science Inc.), Tibor Torok (Predictive Science Inc.), Viacheslav TitovView More
Authors: Talwinder Singh (The University of Alabama in Huntsville), Christian Hall (The University of Alabama in Huntsville), Timothy Newman (The University of Alabama in Huntsville),View More
Authors: Roger Pujadas i Rello (NASA GSFC), Teresa Nieves-Chinchilla (NASA GSFC) A flux rope is a structure in the Sun’s atmosphere, comprising twisted magnetic fieldView More
Authors: Mariana Jeunon (NASA GSFC/CUA), Sanchita Pal (NASA GSFC/GMU), Fernando Carcaboso (NASA GSFC), Teresa Nieves-Chinchilla (NASA GSFC), Georgia De Nolfo (NASA GSFC), Eric Christian (NASAView More
Authors: D.I. Pontin (University of Newcastle, Austrlia), E.R. Priest (University of St Andrews, UK), L.P. Chitta (Max Planck Institute for Solar System Research), V.S. TitovView More
Authors: Chris R. Gilly (Southwest Research Institute), Chris Lowder (Southwest Research Institute), Craig Deforest (Southwest Research Institute) The FLUX code uses a pseudo-lagrangian framework toView More
Authors: Westlake, J.H. (JHU/APL), D.J. McComas (Princeton University), E. Christian (GSFC), N. Schwadron (UNH), and the IMAP Team The Interstellar Mapping and Acceleration Probe (IMAP)View More
Authors: Alexandre Brosius (Penn State/GSFC), Tim Kane (Penn State), Jaye Verniero (GSFC) Current sheets are a universal feature of space plasmas, yet they are notView More
Authors: A. Mubashir(Georgia State University), A. Ashok(Georgia State University), A.G. Bourgeois(Georgia State University), Y.T. Chien(Georgia State University), M. Connors(Georgia State University), E.Potdevin(Georgia State University), X.View More
Authors: Wen He (UAH), Qiang Hu (UAH), Ju Jing (NJIT), Haimin Wang (NJIT) Magnetic field plays an important role in various solar eruption phenomena likeView More
Authors: Abdullah Shmies (The University of Texas at San Antonio), Maher A. Dayeh (Southwest Research Institute), Radoslav Bucik (Southwest Research Institute), Samuel T. Hart (TheView More
Authors: Bart van der Holst (University of Michigan), Gabor Toth (University of Michigan), Merav Opher (Boston University) The outer heliosphere model in the Space WeatherView More
Authors: Xiaocan Li (Dartmouth College), Fan Guo (LANL), Yan Yang (University of Delaware), Hui Li (LANL) An intriguing characteristic of 3D reconnection is the presenceView More
Authors: Kyung-Eun Choi(SSL), Oleksiy Agapitov(SSL) Whistler waves in the solar wind are one of the candidates for regulating the solar wind heat flux and scatteringView More
Authors: Malcolm Colson (University of New Hampshire) Earth is constantly being showered with cosmic rays, most of which produce energetic neutrons that can make itView More
Authors: Soumyaranjan Dash (Institute for Astronomy, University of Hawaii at Manoa; CESSI, IISER Kolkata, India), Dibyendu Nandy (CESSI, DPS, IISER Kolkata, India), Ilya Usoskin (SpaceView More
Authors: Bin Zhuang (UNH), Noé Lugaz (UNH), Nada Al-Haddad (UNH), Camilla Scolini (UNH), Charles J. Farrugia (UNH), Florian Regnault (UNH), Emma E. Davies (ASWO), WenyuanView More