K-Coronal Temperatures Eclipse Experiment
Authors: Sarah Bruce (University of Colorado Boulder), Kevin Reardon (National Solar Observatory) During the total solar eclipses of 20 April, 2023 in Exmouth, Australia andView More
Category: 2024 WG1: Solar (including interior) and coronal
SHINE 2024 abstracts associated with WG1
Multi-point constraints to large scale structure evolution
Authors: Yeimy J. Rivera (Center for Astrophysics | Harvard & Smithsonian) A more comprehensive understanding of the formation, development, and evolution of large-scale solar structures,View More
Automatically Labelled EUV and XRay Incident Solarflares (ALEXIS Solar Flare Catalog)
Authors: Jorge Padial (Vanderbilt University), Kelly Holley-Bockelmann (Vanderbilt University), Eric Jonas (University of Chicago) Predicting extreme space-weather events are important to protect the transmission andView More
An Automated Solar Active Region Identification and Characterization Module for the SEPCaster Model
Authors: Sailee Sawant (The University of Alabama in Huntsville), Gang Li, Meng Jin (Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA 94304, USA) ActiveView More
COLLISIONAL SHEARING: A POSSIBLE PROCESS BEHIND RECURRENT EXPLOSIVE ACTIVITY IN SOLAR ACTIVE REGIONS
Authors: Georgios Chintzoglou Solar Active Regions (ARs) are produced by the emergence of strong magnetic fields generated in the solar interior. ARs can be furtherView More
Coronal Currents: What are they good for?
Authors: Peter W. Schuck (NASA/GSFC) Currents are a much maligned observable in solar physics. There are many advantages to understanding solar phenomena through the evolutionView More
Unsupervised Machine Learning to Identify Structures of the Solar Photosphere
Authors: Leah Zuckerman (University of Colorado, Boulder / NSO), Kevin Reardan (University of Colorado, Boulder / NSO) To answer many open questions in solar research,View More
Progress Toward Understanding Impulsive Magnetic Energy Release in Flares & CMEs [Plenary]
Authors: Brian T. Welsch (Univ. Wisc. – Green Bay) Solar flares and coronal mass ejections (CMEs) are manifestations of the sudden release of magnetic energyView More
Magnetic Field-Dependent Inflows towards Active Regions & Their Nonlinear Impact on a 3D Babcock-Leighton Solar Dynamo Model
Authors: Kinfe Teweldebirhan, Mark Miesch, Sarah Gibson The changing magnetic fields of the Sun are generated and maintained by a solar dynamo, the exact natureView More
How Do Spatial Resolution and Cadence Affect the Accuracy of Electric Field and Poynting Flux Inversions?
Authors: Dennis Tilipman (University of Colorado, Boulder / NSO), Maria Kazachenko (University of Colorado, Boulder / NSO / LASP), Matthias Rempel (National Center for AtmosphericView More
How Does Magnetic Twist at the Solar Photosphere Evolve Prior to Large, Eruptive Flares?
Authors: Brian T. Welsch (Univ. Wisc. – Green Bay), Yang Liu (Stanford University) Energy released in solar flares and coronal mass ejections (CMEs) is believedView More
Magnetic Eruption from a Three-ribbon Flare
Authors: Mia Mancuso (NJIT), Ju Jing (NJIT), Jeongwoo Lee (NJIT), Qin Li (NJIT), Nian Liu (NJIT), Yan Xu (NJIT), Haimin Wang (NJIT) We present observationsView More
Initial findings on the presence of a flux rope during the February 15, 2011 coronal mass ejection (CME) eruption, analyzed using the nonlinear force-free field (NLFFF) model
Authors: Amaal Mohamed (Solar Lab., Solar and Space Dept., “NRIAG”, Helwan, Cairo, Egypt, 11421.) The interaction dynamics between coronal holes (CHs) and coronal mass ejectionsView More
Magnetic flux imbalalnce in the coronal holes and their relation with solar wind speed
Authors: Khagendra katuwal, R.T. James McAteer n this work, we focused on studying 70 coronal holes located at the center of the solar disk withinView More
Investigating the Structure and Dynamics of the Heliospheric Current Sheet
Authors: Lizet Casillas (UCLA), Marco Velli (UCLA), Victor Reville (IRAP), Benjamin Lynch (UCLA) The heliospheric current sheet (HCS) is the boundary between open magnetic fieldView More
Advancing Solar Flare Forecasting with Early Signature Detection
Authors: Juan Camilo Buitrago-Casas (SSL – UCB), Marianne Peterson (UMN), Juliana Vievering (APL), P.S. Athiray, Phillip Chamberlin, Lindsay Glesener, Säm Krucker, Andrea Lopez, Courtney Peck,View More
Solar Prominence Instabilities and Evolution Toward Eruptions
Authors: Wei Liu (LMSAL/BAERI), Thomas Berger (Univ. Colorado), Andrei Afanasev (Univ. Colorado), and Yuhong Fan (UCAR/HAO) Solar prominences are large-scale plasma structures embedded in non-potentialView More
Self-consistent Formation and Resistive Instability of a Simulated Flare Current Sheet
Authors: Silvina Guidoni (American University), Rebecca Bonness (American University) During solar eruptions, massive amounts of energy stored in the coronal magnetic field are converted intoView More
Non-adiabatic Shock Heating in Extended Magnetohydrodynamic Models
Authors: Gabor Toth (University of Michigan), Bart van der Holst (University of Michigan), Xiantong Wang (University of Michigan) Extended magnetohydrodynamic (XMHD) involves extra variables and/orView More
SynCOM: A Model for High-Resolution Simulations of Transient Solar Wind Flows
Authors: Valmir Moraes Filho (Catholic University at NASA/GSFC), Vadim Uritsky (Catholic University at NASA/GSFC), Barbara Thompson (NASA/GSFC), Sarah Gibson (UCAR), Craig DeForest (SwRI) The SyntheticView More
Estimating the Maximum Magnetic Energy Storage of AR 11158 prior to its X2.2 Flare
Authors: Jonathan Lee (Institute for Astronomy, University of Hawaii at Manoa), Xudong Sun (Institute for Astronomy, University of Hawaii at Manoa), Tibor Török (Predictive ScienceView More
A Comparative Study on the Divergent Eruptive Behaviors of AR 12192 and AR 13664
Authors: Kara L. Kniezewski (Air Force Institute of Technology), Seth H. Garland (Air Force Institute of Technology) The solar storms in May of 2024 wereView More
Owens Valley Solar Arrays: An Integrated Community Facility for Solar and Space Weather Research
Authors: Bin Chen (NJIT), Dale Gary (NJIT), Gelu Nita (NJIT), Sijie Yu (NJIT), Pascal Saint-Hilaire (UC Berkeley), Gregg Hallinan (Caltech), and the EOVSA and OVRO-LWAView More
Long Term trends in Sun’s Global Flows: Meridional Flow and Torsional Oscillation
Authors: Sushant S. Mahajan (Stanford University) , Lisa A. Upton (Southwest Research Institute), H. M. Antia (UM-DAE Centre of Excellence for Basic Sciences, University ofView More
AWSoM MHD Simulation of a Solar Active Region: Statistical Analysis of Alfven Wave Dissipation and Reflection, Scaling Laws, and Energy Budget on Coronal Loops
Authors: Tong Shi (SETI Institute), Ward Manchester IV (University of Michigan), Enrico Landi (University of Michigan), Bart van der Holst (University of Michigan), Judit SzenteView More
Statistical Survey of Quasi-periodic Fast-mode Propagating Wave Trains (QFPs) Associated with Flares/CMEs in the Solar Corona
Authors: Richard Zhang (Cupertino High School and Stanford University), Wei Liu (Lockheed Martin Solar and Astrophysics Laboratory), Ruizhu Chen (Stanford University) The magnetized solar coronaView More
Sunspot Penumbral Fine-Scale Bright Dots as a Precursor to Coronal Plumes?
Authors: Ayla Weitz (University of Colorado, NSO), Sanjiv Tiwari (LMSAL, BAERI), Bart De Pontieu (LMSAL, University of Oslo), Gianna Cauzzi (NSO), Kevin Reardon (University ofView More
Is the Average Energy Deposition Rate in Open Field Regions Constant?
Authors: Zhenguang Huang (University of Michigan), Gabor Toth (University of Michigan), Nishtha Sachdeva (University of Michigan), Bart van der Holst (University of Michigan), and WardView More
Unveiling the uniqueness of small-scale solar flare precursors
Authors: Karin Dissauer (NorthWest Research Associates, 3380 Mitchell Lane, Boulder, CO 80301, USA), KD Leka (NorthWest Research Associates, 3380 Mitchell Lane, Boulder, CO 80301, USA,View More
Multi-Spacecraft Analysis of 3D-Trajectory of Blobs in the Solar Corona
Authors: C. López-Portela (GSFC; Univ. of Baltimore), M. P. Miralles (Center for Astrophysics | Harvard & Smithsonian), A. Lara (Instituto de Geofísica, UNAM) The minimumView More
Solar Flare Prediction using Deep Learning Models
Authors: Joao Felipe Sousa Pereira (George Mason University), Jie Zhang (George Mason University), Liang Zhao (Emory University), Dazhou Yu (Emory University), Suman Dhakal (George MasonView More
Simulation of Coronal Mass Ejection Based on the Titov-Demonlin Model: Flux Rope Insertion, Relaxation, and Eruption Triggered by Flux Cancellation
Authors: Xianyu Liu (University of Michigan), Igor Sokolov (University of Michigan), Tamas Gombosi (University of Michigan) The energy build-up and triggering processes of the coronalView More
Investigating the Role of Diffusivities in Solar Convection Modeling
Authors: Brandon Lazard (Univ. California Los Angeles), Nicholas Featherstone (Southwest Research Institute), Jonathan Aurnou (Univ. California Los Angeles) Convection plays a dominant role in governingView More
CME Precursors in an MHD Eruption Model
Authors: Joel T. Dahlin (University of Maryland), Spiro K. Antiochos (University of Michigan), C. Richard DeVore (NASA Goddard Space Fight Center) Coronal Mass Ejections (CMEs)View More
The Plasma-Prescribed Active Region Extrapolation Dataset
Authors: Nat Mathews (NASA GSFC), Barbara Thompson (NASA GSFC) An increase in machine learning based techniques for solar research has mandated the creation of aView More
Consequences of Fields and Flows in the Interior and Exterior of the Sun (COFFIES)
Poster link: https://helioshine.org/wp-content/uploads/2024/08/SAHW_SHINE_2024_Poster.pdf
Hear the songs of the inner heliosphere recorded by Parker Solar Probe
Authors: Jaye Verniero (NASA GSFC), Robert Alexander (NASA GSFC/UMBC), Kristoff Paulson (SAO), Sam Badman (SAO) Parker Solar Probe (PSP) is sampling unprecedented regions of theView More
Helioseismic Properties of Dynamo Wave Signatures in Solar Zonal Flow
Authors: Krishnendu Mandal (New Jersey Institute of Technology), Alexander G. Kosovichev (New Jersey Institute of Technology, NASA Ames Research Center),Valery V. Pipin (Institute of Solar-TerrestrialView More
The Alfven transition zone observed by the Parker Solar Probe in young solar wind – global properties and model comparisons
Authors: Rohit Chhiber (NASA GSFC & U Delaware), Arcadi Usmanov (NASA GSFC & U Delaware), William Matthaeus (U Delaware), Melvyn Goldstein (SSI), and Others TheView More
Refinement of global coronal and interplanetary magnetic field extrapolations constrained by remote-sensing and in situ observations at the solar minimum
Authors: Guanglu Shi (Purple Mountain Observatory), Li Feng (Purple Mountain Observatory), Beili Ying (Purple Mountain Observatory), Shuting Li (Purple Mountain Observatory), Weiqun Gan (Purple MountainView More