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
Tag: 2022 Session 05. Understanding and Quantifying the Performance and Uncertainties in Solar and Heliospheric Models
Abstracts associated with session 5
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
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
Quantifying the Impacts of Interplanetary Propagation and Transient Events on Solar Energetic Particle Intensity-Time Profiles
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
Integrating automated coronal mass ejection detection alerts from a ground based coronagraph for use in solar energetic particle event forecasting
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
Parametric Decay of Circularly Polarized Alfven Wave: One Dimensional and Multidimensional Simulations
Authors: Noshin Mashayekhizadeh(University of New Hampshire), Benjamin D G Chandran(University of New Hampshire), Kai Germaschewski(University of New Hampshire) In parametric decay, the presence of aView More
Homogenizing Solar Extreme Ultraviolet Imaging Surveys with Uncertainty: A model-ensemble approach
Authors: Subhamoy Chatterjee (SwRI), Andres Munoz-Jaramillo (SwRI), Maher Dayeh (SwRI & UTSA), Hazel Bain (CIRES & NOAA SWPC), Kim Moreland (UTSA & SwRI) Solar imagesView More
Validation of Image Based Method for Optimizing Coronal Magnetic Field Models
Authors: Christopher Rura (the Catholic University of America/NASA GSFC), Vadim Uritsky (the Catholic University of America/NASA GSFC), Shaela Jones (the Catholic University of America/NASA GSFC),View More
Underestimation of the polar magnetic flux mesurements due to projection effects from the ecliptic view and the open flux problem.
Authors: Sajay Gosain, Han Uitenbroek The distribution and evolution of the magnetic field at the solar poles through a solar cycle is an important parameterView More
Energy and Spectral Analysis of an AWSoM MHD Simulated Active Region
Authors: Ward Manchester, Enrico Landi, Tong Shi, Judit Szente, Bart van der Holst, Gabor Toth (University of Michigan) We simulate an active region appearing nearView More
Is the coronal magnetic topology of Potential Field Source Surface models robust to boundary conditions from different Surface Flux Transport models?
Authors: Graham Barnes(NWRA), Marc DeRosa(LMSAL), Shaela Jones(NASA GSFC), Mark Cheung(LMSAL), C. Nick Arge,(NASA GSFC), Carl Henney(AFRL) The geometry, connectivity, and topology of the large-scale coronalView More
Estimating uncertainties in the back-mapping of the fast solar wind
Authors: Alexandros Koukras (KU Leuven, Royal Observatory of Belgium), Laurent Dolla (Royal Observatory of Belgium), Rony Keppens (KU Leuven) Although the most likely source regionsView More
Importance of Understanding the CME Three-Part Structure and Its Implication for the CME Radial Expansion
Authors: Bin Zhuang (University of New Hampshire), Noé Lugaz (University of New Hampshire) The CME three-part structure in white-light images has been studied for decades.View More
MHD Simulation Uncertainties Imposed by Boundary Condition Choices
Authors: Lucas Tarr (National Solar Observatory), Mark Linton (Naval Research Laboratory), Peter Schuck (Goddard Space Flight Center), James Leake (Goddard Space Flight Center) A cruciallyView More
Calibrating the WSA model in EUHFORIA based on PSP observations: challenges and limitations toward the improvement of solar wind forecasting
Authors: Evangelia Samara (Royal Observatory of Belgium, Belgium and KU Leuven, Belgium), Charles N. Arge (NASA/GSFC, USA), Rui F. Pinto (LDE3, Uni. Paris-Saclay, France andView More
Predicting Solar Wind Footpoints as Probability Distributions using WSA/ADAPT
Authors: Daniel da Silva (NASA/GSFC, UMBC), Nick Arge (NASA/GSFC), Shaela Jones (NASA/GSFC, Catholic University), Samantha Wallace (NASA/GSFC) The origin point on the sun corresponding toView More
Classification of Solar Wind Instabilities in the Inner Heliosphere
Authors: Mihailo M. Martinovic (University of Arizona), Kristopher G. Klein (University of Arizona), Tereza Durovcova (Charles University, Prague), Benjamin L. Alterman (Southwest Research Institute) InstabilitiesView More
Double Side Photospheric Flux Transport Model combining Front-side and Far-side Information
Authors: Heinemann S.G (Max Planck Institute for Solar System Research, 37077 Göttingen, Germany), Yang, D. (Max Planck Institute for Solar System Research, 37077 Göttingen, Germany)View More