SHINE 2023 deadlines and website logistics
Welcome to the new SHINE newsletter mail service. You may have noticed many automated emails coming through and we appreciate your patience as we getView More
Author: ktindiana
NASA-NOAA O2R funding opportunity
On March 29, 2023, the Step-1 and Step-2 proposal due dates for B.7 Space Weather Science Application Research-to-Operations-to-Research (SWR2O2R) were deferred to until April 28View More
JOB OPPORTUNITY: Term-limit Civil Servant Research Scientist at NASA Goddard Space Flight Center
Updated April 3, 2023 The Energetic Particle Laboratory at NASA Goddard Space Flight Center has an opening for an early-career scientist interested in the originView More
Call for papers: Energy Transfer And Exchange With Low-Energy Plasma Via Cross-Energy And Cross-Scale Interactions Throughout The Magnetosphere
Dear Colleagues, We would like to invite you to submit a paper to the Frontiers in Astronomy and Space Sciencesspecial issue titled “Energy Transfer And ExchangeView More
SHINE 2023 Session Proposal Deadline Extended
Please submit your 2023 SHINE session proposal at the following link: https://forms.gle/onZN3Q7evbAmxxeS8 2023 SHINE Workshop Session Proposals Deadline Extended to March 3rd The 2023 SHINEView More
Call for SHINE 2023 Session Proposals
Dear SHINErs, Please see two announcements below. Noé Lugaz, on behalf of the SHINE steering committee. 1- 2023 SHINE Workshop Session ProposalsThe 2023 SHINE workshopView More
High frequency wave power in the chromosphere – comparison of observations with 3D models
Authors: Momchil Molnar (APS, LASP, University of Colorado, Boulder/NSO), Kevin Reardon (University of Colorado, Boulder/NSO), Steven Cranmer (APS, LASP,University of Colorado, Boulder), Adam Kowalski (APS,View More
Deriving Magnetic Reconnection Rate in the M6.5 Flare on 2015 June 22 With Highest Spatial Resolution
Authors: Bryce Cannon (NJIT), Haimin Wang (NJIT), Ju Jing (NJIT) Magnetic reconnection is an important process to quickly release stored magnetic energy in solar flares.View More
Full disk spectropolarimetry using a multi-slit spectrometer
Authors: Alexandra Glenn (UH Mānoa, IfA), Haosheng Lin (UH Mānoa, IfA) SPIES mock-up is a proof of concept instrument that will prove the viability ofView More
Magnetic field of CMEs as represented by 40+ years of analyses
Authors: Nada Al-Haddad (SSC, UNH), Noé Lugaz (SSC, UNH) Magnetic field structure of Coronal Mass Ejections has been often thought of as accurately represented byView More
Arbitrary open boundary conditions for data driven magnetohydrodynamic simulations: validation using an expanding spheromak ground truth simulation
Authors: Lucas A. Tarr (NSO), Dylan Kee (NSO), Mark Linton (NRL), Peter Schuck (GSFC), James Leake (GSFC) We present a method to formulate numerical boundaryView More
Bystander Training
Attendees of the SHINE workshop are asked to sign up for Bystander Training from Step Up! Step UP! is an award winning, evidence-based bystander interventionView More
Identifying Circularly-Polarized Waves in the Solar Wind Using 1D Convolutional Neural Networks
Authors: Samuel Fordin (University of Delaware),Michael Shay (University of Delaware),Lynn B. Wilson III (NASA GSFC),Bennett Maruca (University of Delaware),Barbara Thompson (NASA GSFC) 26 years ofView More
Nature and Scalings of Density Fluctuations of Compressible MHD Turbulence with Applications to the Solar Wind
Authors: Xiangrong Fu (New Mexico Consortium), Hui Li (Los Alamos National Laboratory), Zhaoming Gan (New Mexico Consortium), John Steinberg (Los Alamos National Laboratory) The solarView More
Strong Alfven Wave Interactions in a Laboratory Plasma
Authors: M. Abler (Space Science Institute), S. Dorfman (Space Science Institute), C.H.K. Chen (Queen Mary University of London) A problem of interest in solar windView More
Opportunities for the study of heliospheric and astrophysical plasmas at the Wisconsin Plasma Physics Laboratory
Authors: Joseph Olson (UW-Madison), Cary Forest (UW-Madison), Jan Egedal (UW-Madison), John Sarff (UW-Madison) The Wisconsin Plasma Physics Laboratory (WiPPL) is a multi-machine, collaborative research facilityView More
How would CMEs with different magnetic morphologies appear in heliospheric white-light imaging?
Authors: Provornikova, E. (JHU APL), Malanushenko, A. (NCAR, HAO), Vourlidas, A. (JHU APL), Gibson, S. (NCAR, HAO), Merkin, V.G. (JHU APL), C. N. Arge (NASAView More
Algorithmically Identifying Upflows and Downflows in the Solar Chromosphere and Transition Region using IRIS MgII Observations
Authors: Vicki Herde (LASP), Phil Chamberlin (LASP), Don Schmit (LASP), Vanessa Polito (BAERI), Ryan Milligan (QUB), Adrian Nigel (GSFC) It’s well-known that the Solar coronaView More
On the Sun’s faintest coronal hard X-rays
Authors: Juan Camilo Buitrago-Casas (UC Berkeley), Lindsay Glesener (University of Minnesota), Steven Christe (NASA GSFC), Säm Krucker (UC Berkeley), Juliana Vievering (Applied Physics Laboratory JohnsView More
Improving Solar Wind Predictions Using Multi-Satellite In Situ Observations
Authors: Dinesha V. Hegde (Department of Space Science & Center for Space Plasma and Aeronomic Research (CSPAR), The University of Alabama in Huntsville, Huntsville, ALView More
Predicting Magnetic Chirality of Coronal Mass Ejections and Potential Geoeffectiveness of Solar Storms
Authors: Lizet Casillas Coronal Mass Ejections (CMEs) can create powerful magnetic storms that can have devastating effects on earth environment as they affect satellites, powerView More
Effects of heliosphere plasma conditions on the properties of astrophysical dust grains
Authors: André Nicolov (Caltech), Paul Bellan (Caltech) When surrounded by plasma, astrophysical dust acquires charge through collisions with electrons. The dust-plasma system is governed byView More
Anterograde Collisional Analysis of Solar Wind Ions
Authors: Elliot Johnson The solar wind is ejected out of the Sun at high temperatures and is moving at a high speed, it is not inView More
Abstract Submission Deadline Extended
Workshop Dates: June 27 to July 1, 2022 (back-to-back with GEM)Joint GEM-SHINE Day: Saturday-Sunday, June 25-26 The GEM-SHINE joint meeting will be held Saturday and Sunday June 25 andView More
SHINE Newsletter 2022-05-29
Workshop Dates: June 27 to July 1, 2022 (back-to-back with GEM)Joint GEM-SHINE Day: Saturday-Sunday, June 25-26 The GEM-SHINE joint meeting will be held Saturday and Sunday June 25 andView More
Developing the Michigan Sun-to-Earth Model
Authors: Gabor Toth (University of Michigan) As part of the Space Weather with Quantified Uncertainty program, our project, funded by NSF, has been working onView More
Modeling of Multiscale Solar Dynamics for Understanding Drivers of Space Weather
Authors: I. Kitiashvili (NASA Ames Research Center), A. Wray (NASA Ames Research Center), V. Sadykov (Georgia State University), A. Kosovichev (New Jersey Institute of Technology/NASAView More
Analysis of Solar Flare Observations obtained by the MinXSS-1 CubeSat
Authors: Christopher S. Moore (Harvard|Smithsonian Center for Astrophysics), MinXSS Team Solar flares accelerate particles on timescales of minutes, converting magnetic energy to thermal, radiative andView More
The Origin of Fe-rich Gradual Solar Energetic Particle Events
Authors: Nariaki Nitta (LMSAL), Meng Jin (SETI/LMSAL), Christina Cohen (Caltech) In the commonly used classification scheme of solar energetic particle (SEP) events, particles in gradualView More
Improving Space Weather Predictions with Data-driven Models of the Solar Atmosphere and Inner Heliosphere
Authors: N.V. Pogorelov (University of Alabama in Huntsville), C.N. Arge (NASA Goddard Space Flight Center), P.C. Colella (Lawrence Berkeley National Laboratory), J. Linker (Predictive ScienceView More
Turbulent properties of the solar wind within corotating interaction regions: superposed epoch analysis of simulations and observations
Authors: Keyvan Ghanbari (University of Alabama in Huntsville), Vladimir Florinski ( the university of Alabama in Huntsville), Gary P. Zank ( the university of AlabamaView More
The Vector Tomographic Inversion for the Solar Coronal Magnetic Field with DKIST and UCoMP instruments.
Authors: Maxim Kramar (University of Hawaii at Manoa), Haosheng Lin (University of Hawaii at Manoa) The coronal magnetic field is important driving force for transientView More
Nowcasting and forecasting SEP events with the iPATH model
Authors: Junxiang Hu (UAH), Gang Li (UAH) This work showcases the nowcasting and forecasting capabilities of the operational version of the iPATH (improved Particle AccelerationView More
Multi-flare analysis of the chromospheric 3-minute oscillations
Authors: Laurel Farris (New Mexico State University), Sean Sellers (New Mexico State University), James McAteer (New Mexico State University) The 3-minute oscillations that dominate theView More
Properties of Forbush Decreases observed with the AMS-02 daily proton flux
Authors: Veronica Bindi (University of Hawaii at Manoa), Cristina Consolandi (University of Hawaii at Manoa), Claudio Corti (University of Hawaii at Manoa), Chris Light (UniversityView More
Magnetic Reconnection and Energy Partition in Three-dimensional Plasma Turbulence
Authors: Yi-Hsin Liu (Dartmouth College), Yi Qi (University of Colorado Boulder), and C. T. Russell (UCLA) What mechanisms dissipate energy in plasma turbulence is anView More
FETCH concept: Investigating Quiescent and Transient Magnetic Structures in the Inner Heliosphere using Faraday Rotation of Spacecraft Radio Signals
Authors: Megan Kenny (University of Colorado, Boulder) Liz Jensen (Planetary Science Institute) Shing F. Fung, Lynn Wilson III, Lan Jian, Nat Gopalswamy, Teresa Nieves-Chinchilla (HeliophysicsView More
Thermal Analysis of the Plasma Sheet Region
Authors: DeOndre Kittrell (NASA GSFC), Katharine Reeves (Harvard-Smithsonian Center for Astrophysics We conduct detailed thermal analysis of the plasma sheet region during the post-eruption phaseView More
CHMAP: Coronal Hole Mapping and Analysis Pipeline
Authors: James Turtle (PSI), Cooper Downs (PSI), Opal Issan (PSI), Tamar Ervin (PSI), Ronald M. Caplan (PSI), Jon A. Linker (PSI) Since the launch ofView More
Guide field dependence of energy spectrum and energy transfer in reconnection
Authors: Michael Shay(University of Delaware), Tulasi N. Parashar (Victoria University of Wellington), William H. Matthaeus (University of Delaware) Classic picture of magnetic reconnection has shownView More