Using Magnetic Flux Conservation to Determine Heliosheath Speeds
Authors: John D Richardson MIT Authors C Alan C Cummings CALTECH B Leonard F Burlaga NASA Goddard Space Flight Center John D RiJ. D. RichardsonView More

Authors: John D Richardson MIT Authors C Alan C Cummings CALTECH B Leonard F Burlaga NASA Goddard Space Flight Center John D RiJ. D. RichardsonView More
Authors: Matthew West (Southwest Research Institute), Federica Frassati (National Institute of Astrophysics – Astrophysical Observatory of Turin), Monica Laurenza (Istituto di Astrofisica e Planetologia Spaziali),View More
Authors: Erick Powell (Boston University), Merav Opher (Boston University), Marc Kornbleuth (Boston University) Neutral hydrogen in the hydrogen wall (beyond the heliopause) and heliosheath absorbView More
Authors: Bryan Yamashiro (University of Hawaii), Xudong Sun (University of Hawaii) The Sun’s polar magnetic fields impart strong constraints on the internal dynamo process, theView More
Authors: Gabor Toth (University of Michigan), Nishtha Sachdeva (University of Michigan), Lulu Zhao (University of Michigan), Bart van der Holst (University of Michigan), Igor SokolovView More
Authors: James Staeben (UVA/NASA GSFC), Nick Arge (NASA GSFC), Shaela Jones (NASA GSFC/CUA) Accurate forecasting of space weather grows increasingly important as we move towardsView More
Authors: Colby C. Haggerty (University of Hawaii, Manoa), Michael Shay (University of Delaware), Tai Phan (University of California, Bekeley), Paul Cassak Magnetic reconnection in currentView More
Authors: Fernando Carcaboso (NASA Goddard Space Flight Center, The Catholic University of America), Raúl Gómez-Herrero (Space Research Group, University of Alcalá), Francisco Espinosa Lara (SpaceView More
Authors: Jacob McLaughlin (University of Iowa), Fred Skiff (University of Iowa) Neutral calcium plasma is particularly interesting for studies of ion wave dynamics. Apart fromView More
Authors: Tom Schad (National Solar Observatory), Alexandra Tritschler (National Solar Observatory), and the DKIST Science Team The chromospheric and coronal polarimetric capabilities of DKIST, inView More
Authors: Shaheda Begum Shaik (George Mason University), Mark Linton (Naval Research Laboratory), Phillip Hess (Naval Research Laboratory), Sarah Gibson (National Center for Atmospheric Research) WeView More
Authors: Chen Shi (UCLA), Marco Velli (UCLA), Anna Tenerani (UT Austin), Anton Artemyev (UCLA) The stability problem of current sheets is one of the mostView More
Authors: Luiz F. G. dos Santos (nextSource Inc), Thomas Narock (Goucher College), Ayris Narock ( NASA GSFC/ADNET Systems Inc), Sanchita Pal (NASA GSFC/University of Helsinky),View More
Authors: M. A. Dayeh (SwRI), M. J. Starkey (SwRI), R. Bučik (SwRI) and M.I. Desai (SwRI) The interplanetary Suprathermal (ST) ion population is unambiguously thoughtView 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: Chen Shi (UCLA), Marco Velli (UCLA), Anna Tenerani (UT Austin) Solar wind is highly turbulent and contains fluctuations on all scales which are dynamicallyView More
Authors: Kai Yang (Institute for Astronomy, University of Hawaii at Manoa) Magnetic helicity is conserved under ideal magnetohydrodynamics and quasi-conserved even under a resistive process.View More
Authors: Chika Onubogu (Boston University), Merav Opher (Boston University), Marc Kornbleuth (Boston University) The properties of the solar wind vary with the solar cycle, evolvingView More
Authors: Alberto Sainz Dalda (BAERI/LMSAL) This session will start with a critical review of the usage of machine learning (ML) and data assimilation (DA) inView More
Authors: F. Fraternale (University of Alabama in Huntsville – CSPAR), R. K. Bera (University of Alabama in Huntsville – CSPAR, USA), N. V. Pogorelov (UniversityView More
Authors: Xiaohan Ma (Boston University), Merav Opher (Boston University) The heliosphere is a vast region surrounding the Sun that marks the outer limits of theView More
Authors: Alicia K. Petersen (Air Force Research Lab, NRC), Stephen M. White (Air Force Research Lab, Kirtland AFB), Stephen W. Kahler (Air Force Research Lab,View More
Authors: Dylan Conner (WVU), Katherine Goodrich (WVU), Justin Bowman (WVU), Justin Riggs (WVU) Parker Solar Probe, while engaging in a gravity assist maneuver with Venus,View More
Authors: Ashraf Moradi (University of Arizona), Joe Giacalone (University of Arizona) Solar protons with rigidities higher than 1 GV (432 MeV) penetrate Earth’s atmosphere, generateView More
Authors: Benjamin Boe (NSF Postdoctoral Fellow. Institute for Astronomy, University of Hawaii), Shadia Habbal (Institute for Astronomy, University of Hawaii), Cooper Downs (Predictive Science Inc.),View More
Authors: Ruizhu Chen (Stanford University), Junwei Zhao (Stanford University), Shea A. Hess Webber (Stanford) The Sun’s far-side magnetic field is important for space weather forecastingView More
Authors: Nicolas Donders (The University of Alabama in Huntsville, Department of Space Science and The Center for Space Plasma and Aeronomic Research), Amy Winebarger (NASAView More
Authors: Sherry Chhabra (George Mason University, Fairfax, VA), Jeffrey Reep (Naval Research Laboratory, Washington DC), Harry Warren (Naval Research Laboratory, Washington DC), N.P.S. Mithun (PhysicalView More
Authors: Nat Gopalswamy (NASA/GSFC) and the MOST team The Multiview Observatory for Solar Terrestrial Science (MOST) is envisioned as the next generation great observatory toView More
Authors: Heather Elliott, John Richardson, George Livadiotis, Tae Kim, Dave McComas, Eric Zirnstein, Pawel Swaczyna, Alan Stern, Randy Gladstone, Pontus Brandt, Fran Bagenal, Matt Hill,View More
Authors: Xiaohang Chen (University of Arizona), Athanasios Kouloumvakos (APL, Johns Hopkins University), Joe Giacalone (University of Arizona), Alexis Rouillard (CNRS) We simulate the spatial andView More
Authors: Joan Burkepile (High Altitude Observatory HAO), Steven Tomczyk (HAO), Ben Berkey (HAO), Marc Cotter (HAO) , Michael Galloy (HAO), Sarah Gibson (HAO), Don KolinskiView More
Authors: Chris R. Gilly (LASP) When SOHO was launched it included a suite of three coronagraphs, C1, C2, and C3. These imagers were made toView More
Authors: Aditya Gandhi (University of Michigan), Mojtaba Akhavan-Tafti (University of Michigan) Magnetic switchbacks, designated by abrupt reversals in the radial component of the magnetic field,View More
Authors: F. Regnault (Space Science Center, Institute for the Study of Earth, Oceans, and Space, University of New Hampshire), N. Al-Haddad (Space Science Center, InstituteView More
Authors: M. D. Galloy (HAO Boulder, CO), J. T. Burkepile (HAO Boulder, CO), M. L. Mays (NASA GSFC), J. T. Jones (NASA GSFC), O. C.View More
Authors: M. Kenny (University of Colorado, Boulder), C. E. DeForest (Southwest Research Institute), P. C. Liewer (Jet Propulsion Laboratory), M. J. West (Southwest Research Institute)View More
Authors: Austin Brenner (University of Michigan), Matti Ala-Lahti (University of Michigan), Tuija Pulkkinen (University of Michigan) When an interplanetary coronal mass ejection impacts the earth’sView More
Authors: Gang Li (University of Alabama in Huntsville), Meng Jin (SETI), Zheyi Ding (KU LEUVEN) In forecasting SEP events, confidence level is an essential aspect. View More
Authors: John Stefan (NJIT), Alexander Kosovichev (NJIT), Andrey Stejko (NJIT) Past studies have found strong deviations in the mean phase travel time of acoustic wavesView More