Abstract associated with student poster for SHINE 2023
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: 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: 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: 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: S. Roy (Center for Astrophysics | Harvard & Smithsonian), K. Reeves (Center for Astrophysics | Harvard & Smithsonian), C. Moore (Center for Astrophysics |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: 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: 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: Shan-Chang Lin (Dartmouth College), Yi-Hsin Liu (Dartmouth College), Xiaocan Li (Dartmouth College) Using 2-dimensional(2D) magnetohydrodynamics (MHD) simulations, we show that Petschek-type magnetic reconnection canView More
Authors: William Ryan (West Virginia University), Paul Cassak (West Virginia University), Vadim Roytershteyn (Space Science Institute), M. Hasan Barbhuiya (West Virginia University), Subash Adhikari (WestView More
Authors: Megan Kenny(1), Craig DeForest(2), Sam Van Kooten(3) The Wide-field Imager for Parker Solar Probe (WISPR) images the inner heliosphere as Parker Solar Probe (PSP)View More
Authors: Aniket Jivani (University of Michigan), Hongfan Chen (University of Michigan), Xun Huan (University of Michigan), Yang Chen (University of Michigan), Bart van der HolstView More
Authors: Christopher Rowell, Dr. Ming Zhang Solar wind parameters are continuously monitored by spacecraft orbiting Earth. It is desirable to know when a solar windView More
Authors: Hasith Perera (West Virginia University),Paul Cassak (West Virginia University),Hasan Barbhuiya (West Virginia University),Greg Howes (University of Iowa) A forefront area of research in weaklyView More
Authors: Razieh Ghamari (University of Delaware), John Clem (University of Delaware), Paul Evenson (University of Delaware), Pierre-Simon Mangeard (University of Delaware), Chanoknan Banglieng (Rajamangala UniversityView More
Authors: Lizet S. Casillas (UCLA), Marco Velli (UCLA) The heliospheric current sheet (HCS) is the boundary between open magnetic field lines of opposite polarity inView More
Authors: Paria Abouhamzeh (Department of Space Science, University of Alabama in Huntsville), Bingbing Wang (The Center for Space Plasma and Aeronomic Research, University of AlabamaView More
Authors: Sahanaj Aktar Banu (University of New Hampshire, Durham, New Hampshire, United States), Reka Winslow (University of New Hampshire, Durham, New Hampshire, United States), EmmaView More
Authors: Joshua Morgan (Caltech), Paul Bellan (Caltech) The Caltech MHD Plasma Jet experiment generates a relatively low temperature plasma of approximately 2eV and density ofView More
Authors: Rayta A. Pradata (University of Delaware), Gang Kai Poh (NASA GSFC/Catholic University of America), Ana Peruza (George Mason University), Zhenguang Huang (University of MichiganView More
Authors: Theodore Broeren (University of Arizona), Kristopher Klein (University of Arizona) The upcoming NASA mission HelioSwarm will use nine spacecraft to make simultaneous measurements ofView More
Authors: Samuel Evans (Boston University Center for Space Physics), Meers Oppenheim (Boston University Center for Space Physics), Juan Martínez-Sykora (Lockheed Martin Solar & Astrophysics Laboratory),View More
Authors: Michael Nastac (University of Oxford), Michael Barnes (University of Oxford), Robert Ewart (University of Oxford), James Juno (Princeton Plasma Physics Laboratory), Alexander Schekochihin (UniversityView More
Authors: Hasan Barbhuiya (West Virginia University), Paul Cassak (West Virginia University) Energy conversion in collisionless space plasmas has garnered significant attention in recent years. KineticView More
Authors: Oliver E. K. Rice (Durham University), Anthony R. Yeates (Durham University) We investigate which scalar quantity or quantities can best predict the loss ofView More
Authors: Yu Xu (Peking Univeristy), Hui Tian (Peking University), Julián Alvarado-Goméz (Astrophysics Institute Potsdam) Coronal mass ejections (CMEs) on the hosting stars are considered toView More
Authors: Zihao Yang (Peking University; NCAR/HAO), Hui Tian (Peking University), Yu Xu (Peking University), Xianyu Liu (Peking University) Coronal mass ejections (CMEs) are the largest-scaleView More
Authors: Niranjana Shankarappa (University of Arizona), Kristopher Klein (University of Arizona), Mihailo Martinovic (University of Arizona) Solar wind heating and acceleration is a long-standing problemView More
Authors: Minami Yoshida (The University of Tokyo, ISAS/JAXA), Toshifumi Shimizu (ISAS/JAXA, The University of Tokyo), Shin Toriumi (ISAS/JAXA) The “open” magnetic field extending from theView More
Authors: Jada Walters (University of Arizona), Kris Klein (University of Arizona), James Juno (Princeton Plasma Physics Laboratory), Jason TenBarge (Princeton University), Emily Lichko (University ofView More
Authors: Lidiya Y. Ahmed1,2 , Michael L. Stevens1, Kristoff Paulson1, Anthony Case1 1 Smithsonian Astrophysical Observatory 2 Harvard University Solar wind parameters such as density,View More
Authors: Kelly Victor-French (NRL), Karl Battams (NRL), Brian Wood (NRL) We present our investigation into the relationship between coronal brightness and the eruptivity of solarView More
Authors: Tania Varesano (SwRI), Donald Hassler (SwRI) We present an analysis of the first connection mosaic made by the SPICE instrument on board of theView More