Predictive Science Inc., California
Parent Institutions [?]
Child Institutions [?]
Affiliated Works
sorted by decreasing year, and then by display-name
- Comparing Eclipse Observations of the August 1, 2008 Solar Corona with an MHD Model Prediction
- Global MHD Modeling of the Solar Corona and Inner Heliosphere for the Whole Heliosphere Interval
- Is Disconnection Necessary?
- Slip-Squashing Factors as a Measure of Three-Dimensional Magnetic Reconnection
- Small Bipoles Interacting with a Coronal Hole: MHD Simulations
- CORHEL: A Modeling Suite for Describing the Solar Corona and Inner Heliosphere
- Comparing High-Resolution MHD Simulations of the Present and Preceding Solar Minima
- Evolution of CMEs in the Heliosphere at Solar Minimum
- Implications of the Deep Minimum for Slow Solar Wind Origin
- Investigating the Topology of the “Disconnection” of Coronal Holes
- MHD Simulations of the Interaction of Small Polarities in Coronal Holes
- On the Relationship Between Coronal Heating, Magnetic Flux, and the Density of the Solar Wind
- 3D Study of Solar Eruptions Using SDO and STEREO Observations
- A Parametric Study to Constrain Empirically-based Models of the Ambient Solar Wind
- Comparing an MHD Model of the Corona During the July 11, 2010 Total Solar Eclipse with Observations (Invited)
- Initiation and Evolution of Corotating Interaction Regions
- Magnetic Maps and Coronal/Solar Wind Modeling: Practices and Pitfalls (Invited)
- Structure and Dynamics of the Erupting Magnetic Flux in the May 12 1997 CME Event
- Temporal evolution and spatial variation of the solar wind from multi-spacecraft measurements
- The Wide Field Imager for Solar PRobe (WISPR)
- Thermal Nonequilibrium Revisited: a Heating Model for Coronal Loops
- Writhing and rotation of erupting prominences and CMEs
- 3D Solar Wind Structure Features Characterizing the Rise of Cycle 24
- Advances in Modeling the initiation and evolution of CMEs through the Solar WInd
- Comparing MHD Simulations of the Solar Corona and the Solar Wind with Data
- Evolution of Electric Currents during Active Region Formation
- How do Heliospheric Remote-Sensing Observations Limit Magnetic Flux Rope Models?
- MHD Modeling of the Sympathetic Eruptions Observed on August 1, 2010
- Magnetic Topology of the Sympathetic CMEs Observed on 27 July 2011 and 1 August 2010
- Observations of the White Light Corona from Solar Orbiter and Solar Probe Plus
- The Rising Phase of Solar Cycle 24: General Solar Wind, Large-Scale Solar Wind Structures, and Sector Asymmetry
- The Unusual Minimum Preceding Cycle 24: What MHD Models Reveal
- Interaction of Cometary Material With the Solar Corona: EUV Observations and MHD Simulations
- Magnetohydrodynamic Simulations of Interplanetary Coronal Mass Ejections
- New Tools to Discover the Physical Links From CME Eruptions to Radiation Effects in Deep Space: a First in Heliospheric End-to-End Coupling
- Prediction of the Solar Corona for the 2012 November 13 Total Solar Eclipse
- Pseudo-Streamer Magnetic Topologies in the 2010 August 1-2 CMEs
- The Day the Sun Stood Still: Using global Thermodynamic MHD Simulations to Infer the Structure of the Solar Corona and Inner Heliosphere during the Maunder Minimum
- The Interaction of Comet C/2011 W3 (Lovejoy) with the Global Solar Corona: Insight and Perspectives from Realistic Thermodynamic MHD Simulations
- The S-Web Hypothesis: Modeling and Observational Challenges
- The Solar Wind From Pseudostreamers And Their Immediate Environment
- Using multi-wavelength observations to constrain CME simulations
- A 3D MHD Model of the Solar Wind Driven by Turbulence Dissipation
- Closed Field Coronal Heating Models Inspired by Wave Turbulence
- Driving Coronal MHD Simulations with Flux Evolution Models
- Embedding Circular Force-Free Flux Ropes in Potential Magnetic Fields
- MHD Modeling of the Sympathetic Eruptions Observed on August 1, 2010
- Particle Acceleration in the Low Corona Over Broad Longitudes: Coupling Between 3D Magnetohydrodynamic and Energetic Particle Models
- Stability of High-energy Coronal Magnetic Fields
- The Quasi-Annual Forcing of The Sun's Eruptive, Radiative, and Particulate Output
- The role of the large-scale coronal magnetic field in the eruption of prominence/cavity systems
- Thermodynamic MHD Simulation of the July 14, 2000, "Bastille Day" Solar Eruption
- Understanding the Evolution of the July 23, 2012 Extreme ICME: Global Modeling and Comparison with Observations
- Characterizing a Model of Coronal Heating and Solar Wind Acceleration Based on Wave Turbulence.
- Constructing Time-Dependent Coronal Hole Maps Using Synchronized Multi-Instrument EUV Data
- Coronal Magnetism: Hanle Effect in UV and IR Spectral Lines
- Coronal Modeling with Flux-Evolved Maps: Comparison with Observations
- How Well Does the S-Web Theory Predict In-Situ Observations of the Slow Solar Wind?
- Magnetic Topology of the Global MHD Configuration on 2010 August 1-2
- Particle Acceleration in the Low Corona Over Broad Longitudes: Coupling MHD and 3D Particle Simulations
- Propagation and Evolution of Interplanetary Magnetic Clouds: Global Simulations and Comparisons with Observations
- Sympathetic solar eruptions in quadrupolar magnetic configurations
- The Solar Energetic Particle Event on 2013 April 11: An Investigation of the Solar Origin of its Longitudinal Widespread
- Time lags of Hinode/XRT and SDO/AIA lightcurves from simulations of impulsive heating
- Time-Dependent Coupling of Lfm-Helio and MAS Models for CME Propagation
- Towards a Thermodynamic 3D MHD Model of Coronal Jets
- Validation of Coronal and Heliospheric Models for Quasi-Steady Solar Wind: WSA-Enlil, MAS-Enlil, SWMF, and IPS Tomography Models
- Vision for the Future of Lws TR&T
- 3D electron density distributions in the solar corona during solar minima: assessment for more realistic solar wind modeling
- Coupling MHD Simulations of CMEs to SEP Models
- Diagnosing the Properties of the Solar Wind using Magnetic Topology
- Fast Wave Trains Associated with Solar Eruptions: Insights from 3D Thermodynamic MHD Simulations
- Flare-associated Fast-mode Coronal Wave Trains Discovered by SDO/AIA: Physical Properties and Implications
- Full-sun synchronic EUV and coronal hole mapping using multi-instrument images: Data and software made available
- How Much Energy Can Be Stored in Solar Active Region Magnetic Fields?
- How Reliable Is the Solar Wind Prediction from the Models Installed at the CCMC?
- Longitudinal Properties of a Widespread Solar Energetic Particle Event on 2014 February 25: Evolution of the Parent CME and Associated Shock
- On the Log-Normality of Historical Magnetic-Storm Intensity Statistics: Implications for Extreme-Event Probabilities
- Predicting the Interplanetary Magnetic Field using Approaches Based on Data Mining and Physical Models
- Slip versus Field-Line Mapping in Describing 3D Reconnection of Coronal Magnetic Fields
- Slow Solar Wind: Observable Characteristics for Constraining Modelling
- Structure, Stability and Evolution of a Magnetic Flux Rope
- Thermodynamic MHD Simulations of Jets in the Solar Corona and Inner Heliosphere
- Time-dependent global modeling of the inner heliosphere
- a Roadmap to Advance Understanding of the Science of Space Weather
- A Free Database of Auto-detected Full-sun Coronal Hole Maps
- A Thin-Flux-Rope Approximation as a Basis for Modeling of Pre- and Post-Eruptive Magnetic Configurations
- Connectivity Between Solar Energetic Particle Observations and Their Solar Sources: The Event on 14 August 2010
- Core Dimming Regions as Probes of Magnetic Connectivity and Reconfiguration.
- Data-Driven Models of the Solar Corona and Solar Wind
- Fundamental Physics of the Slow Solar Wind - What do we Know?
- Identifying "Carrington Events" in Solar, Solar Wind, and Magnetospheric Data
- Magnetic Source Region Characteristics Influencing the Velocity of Solar Eruptions in the Corona
- Observations and Modeling of Plasma Waves in the Solar Atmosphere
- On the Geo-effectiveness of Shocks and Sheaths
- Q-Maps: A New Synoptic Data Product for Investigating Dynamic Coronal Connectivity
- Radiation Environments for Future Human Exploration Throughout the Solar System.
- Sun-to-Earth MHD Modeling of Powerful Solar Eruptions
- The Connection Between the Longitudinal Extent of SEP Events and the Properties of Coronal Shocks
- The Impact of Coronal Jets on the Solar Wind and Magnetic Structures in the Inner Heliosphere.
- The extreme space weather event of 1859: A case of historical and physical alignment
- Tracking Changes in Magnetic Topology in MHD Simulations
- 3D MHD Modeling of Prominence Formation by Plasma Evaporation and Condensation
- An Observational Approach toward Understanding and Prediction of CME Magnetic Ejecta
- Assessing Space Weather Applications and Understanding: IMF Bz at L1
- Can Polar Fields Explain Missing Open Flux?
- Combining Remote and In Situ Observations with MHD models to Understand the Formation of the Slow Solar Wind
- Digging into the corona: A modeling framework trained with Sun-grazing comet observations
- Ion Charge States in the July 14, 2000 CME: MHD Simulations
- Modeling the 21 August 2017 Total Solar Eclipse: Prediction Results and New Techniques
- Predicting SPE Fluxes: Coupled Simulations and Analysis Tools
- Predicting the Magnetic Properties of ICMEs: A Pragmatic View
- Regularized Biot-Savart Laws for Modeling Magnetic Configurations with Flux Ropes
- The Solar Orbiter Heliospheric Imager (SoloHI) for the Solar Orbiter Mission
- The Solar Wind from Pseudostreamers and their Environs: Opportunities for Observations with Parker Solar Probe and Solar Orbiter
- The Wide-Field Imager for the Parker Solar Probe Mission (WISPR)
- The spatial gradients in the solar wind and IMF in the vicinity of the first Lagrangian point
- Thermal energy creation and transport and X-ray/EUV emission in a thermodynamic MHD CME simulation
- COSPAR International Space Weather Action Teams: Coordinated Research Initiative Targeting Improvements of Global Resilience to Space Weather Impacts
- Conjoined Flux Ropes: A New Mechanism for Filament-Channel Formation at External Polarity Inversion Lines
- Coronal Hole Obscuration and Open Flux
- Encounters of Coronal Jets with Parker Solar Probe and Solar Orbiter
- Ensemble approaches to forecasting the near-Earth solar wind
- Exploration of Different Active Region Heating Models
- Formation of a Kilogauss Magnetic Flux Rope Prior to an X9-Class Flare
- Global Coronal Models and Forward Modeling: Connecting Observables to the Underlying Physical State of the Corona
- In Situ Categorization and Coronal Origins of Different Slow Solar Wind Types
- MHD Modeling of the Solar Corona for the Parker Solar Probe First Perihelion Encounter
- Magnetic Energy Bounds for Major Solar Eruptions
- Modeling Pseudo-Streamers with Embedded Magnetic Flux Ropes
- The 2017-Sep-10 EUV Wave and Its Implications for Global Coronal Seismology
- Community-wide Space Weather Scoreboards: Facilitating the Validation of Real-time CME, Flare, and SEP Forecasts
- Comparison of Parker Solar Probe Observations during First Perihelion with Global Magnetohydrodynamic Model Results
- Cooling Condensation at Coronal Null Points and Quasi-Separatrix Layers Involving Magnetic Reconnection
- Data-Constrained Modeling of Eruptions in the Solar Corona: Insights from 3D MHD Simulations
- Deriving the Electron Energy Distribution in the SEP-associated Radio CME of 2012 July 17
- Global Magnetohydrodynamics Simulation of EUV Waves and Shocks from the X8.2 Eruptive Flare on 2017 September 10
- Imaging the Solar Corona from Within: First Results from the Parker Solar Probe Telescope
- International Scientific Coordination on Space Weather: A COSPAR Panel on Space Weather Perspective
- International Scientific Coordination on Space Weather: A COSPAR Panel on Space Weather Perspective
- Modeling Magnetic Flux Ropes with the RBSL Method
- Next Steps for Induced Geo-Electric Fields Benchmarks
- Next Steps in Establishing Benchmarks for Extreme Space Weather
- Prediction of Coronal Structure for the July 2, 2019 Total Solar Eclipse: Comparison with Observations
- Preparing photospheric magnetic field measurements for use in coronal and heliospheric models
- Probing the solar corona with Sun-grazing comets: comparing MHDsimulations with EUV observations
- SPE Threat Assessment Tool (STAT) and Particle Acceleration Resulting from CMEs Modeled from the Photosphere to past 1AU
- Searching for a Boundary Layer as a Source of the Slow Solar Wind
- Showcasing the just released ISWAT website (http://www.iswat-cospar.org) built with a content management platform to serve as an online presence for the ISWAT (International Space Weather Action Teams) - community driven effort hosted by the COSPAR Panel on Space Weather.
- Solar Eruptions Triggered by Flux Emergence
- Stabilities of magnetic flux ropes anchored in the solar surface
- The Solar Orbiter Heliospheric Imager (SoloHI) for the Solar Orbiter Mission: Science and Instrument Status
- Tracking Topological Changes in MHD Simulations using Slip-Back Mapping
- An Adaptive Prediction System for Specifying Solar Wind Conditions Near the Sun
- An Improved Data-Driven Analysis Pipeline for Coronal Hole Detection and Mapping
- CORHEL-Kamodo: PSI tools for the analysis and visualization of MHD models
- COSPAR International Space Weather Action Teams: Addressing Challenges Across the Field of Space Weather.
- Comparing and Contrasting the Three Most Recent Solar Minima using MHD Models
- Coronal Acceleration of Large and Acute SEP Events
- Coronal Prediction for the December 14, 2020 Total Solar Eclipse
- Fine structure of the white-light inner corona and the associated magnetic topology
- Handling the complexity of the space weather system: Novel approaches through particle precipitation and ion outflow
- Kamodo Open Source - A Community Resource for Data and Model Access and an Analysis Library for Space Physics
- Kamodo online visualization at the CCMC
- Linking Magnetic Complexity to Coronal Heating and Solar Wind Structure
- MHD Modeling of an Observed Solar Filament
- Mitigation of Coronal Hole Obscuration for Open Flux Estimates
- Optimization of Magnetic Flux Ropes Modeled with the RBSL Method*
- Partially Open Fields and the Energy of Solar Eruptions
- Solar and Heliospheric Models at the CCMC - An Update
- Two-Temperature, Wave-Turbulence-Driven MHD Simulations of the Solar Corona and the Solar Wind
- A new color-based method for K- and F-corona extraction
- CHMAP: Coronal Hole Mapping and Analysis Pipeline
- Constraining the CME Core's Heating and Energy Budget with SOHO/UVCS
- Coronal Prediction for the December 4, 2021, Total Solar Eclipse
- Evolution of Non-neutralized Electric Currents in Eruptive Solar Active Regions
- Expanding and Testing Orbit Propagation Capabilities Using CCMC-Hosted Models
- Exploring the middle corona: new instrumentation to address science questions critical to understanding the thermal structure and dynamic evolution of the middle corona
- Flux rope reformation as a model for homologous solar flares and coronal mass ejections
- Global MHD Simulations of the Time-Evolving Corona and Heliosphere
- Improving Space Weather Predictions with Data-driven Models of the Solar Atmosphere and Inner Heliosphere
- Kamodo Model Access in Geospace: Use of Custom Readers and Interpolators
- Magnetogram-matching Energization and Eruption of Magnetic Flux Ropes
- Necessary Conditions for a Hot Quiet Sun Atmosphere: Chromospheric Flares and Low Corona Twisted Flux Rope Eruptions
- Open-Source High-Performance Flux Transport
- Partially Open Fields as the Energy Bounds for Solar Eruptions
- Propagation and Deflection of CMEs in Different Background Magnetic Fields
- Quantifying Capabilities in Observing Coronal Mass Ejections
- Shedding light on the evolution of solar transients with multi-spacecraft observations
- Solar Cycle Variability in Coronal Holes and their Effects on Solar Wind Sources
- The COMPLETE mission concept for the Heliophysics Decadal Survey
- Theory and Models of Flare/CME Onset Via Flux Emergence and/or Shear Flows
- Torus-Stable Zone Above Starspots
- Tracing the Drivers of Slow Solar Wind in the Middle Corona
- Tracking and Understanding the Trajectory of CMEs From Birth to Late Stage
- Understanding Solar Eruptions, Solar Wind Formation, and how the Sun Connects to the Heliosphere through a Polar Perspective
- Understanding the coronal origins of global heliospheric phenomena through 3D measurements with COMPLETE
- Validating Numerical WSA Solutions
- Visualization of Space Physics with Kamodo
- Ace in the Hole: The Effect of Time-Dependent Magnetic Fields on Coronal Hole Development
- Applying the RBSL and Helicity-pumping Methods to the Modeling of the 2011 October 1 Pre-eruptive Configuration
- BepiColombo Cruise Science: a Planetary Mission Providing Synergistic Observations of Interplanetary Transients in the Inner Solar System
- Coordinated ground and airborne extended observations of TSE 2024 with Citizen CATE and NASA's WB-57s
- ECCCO: The EUV CME and Coronal Connectivity Observatory
- Estimating the altitude of pulsating aurora emission: triangulation from three ground-based stations during the LAMP rocket experiment
- Following a prominence eruption from the Sun to Parker Solar Probe with multi-spacecraft observations
- LAMP-HEP Observation of Microburst Precipitation associated with Pulsating Aurora
- Modeling CME encounters at Parker Solar Probe with OSPREI: Dependence on photospheric and coronal conditions
- Open-Source High-Performance Flux Transport
- Persistent, Energetic Pulsating Aurora Observed During the LAMP Sounding Rocket Mission Launch Window
- Prominence Eruption Observed in He II 304 Å up to >6 Solar Radii by EUI/FSI Aboard Solar Orbiter
- Quantifying errors in 3D CME parameters derived from synthetic data using white-light reconstruction techniques
- Quantitative Analysis of the Early Trajectory of CMEs in the Inner Corona
- Revisiting the Bastille Day Coronal Mass Ejection: Learning About the Eruption Through 3D MHD Time-Dependent Ionization Modeling of Heavy Ions
- Space Weather Predictions with a New Generation of Data-driven Models of the Solar Atmosphere and Inner Heliosphere: Improving Efficiency and Ensuring Uncertainty Quantification
- Space Weather: Complexity science, convergence research, and a risk and resiliency framework
- Spatial and Temporal Scales of Pulsating Aurora during the Loss Through Auroral Microburst Pulsations (LAMP) Rocket Mission
- The COMPLETE mission concept for comprehensive 3D understanding of coronal magnetic energy storage and release
- The Open Flux Problem: The Need for High Latitude Observations
- The Response of the Corona and of the Heliosphere to Realistic Photospheric Magnetic Flux Evolution
- Visualization Tools for EPREM and Beyond
- Wide energy electron precipitation during pulsating aurora: LAMP sounding rocket experiment and computer simulation
- Widespread SEP Events: Modelling Onsets at Multiple Spacecraft With STAT
Linked Collaborating Authors [?]
- A. J. Halford
- A. K. Higginson
- A. N. Zhukov
- A. W. Case
- Adam Kellerman
- Albert Y. Shih
- Ali Rahmati
- Allison Jaynes
- Amir Caspi
- B. J. Lynch
- Beatriz Sánchez‐Cano
- C. A. Madsen
- C. J. Henney
- C. Kay
- C. M. De Nardin
- C. M. S. Cohen
- Camilla Scolini
- Carolus J. Schrijver
- Christian Möstl
- Christina O. Lee
- Christopher Moore
- Cooper Downs
- D. E. McKenzie
- D. Lario
- Daniel B. Seaton
- Daniel Heyner
- Darren L. De Zeeuw
- Dinesha Vasanta Hegde
- Donald Hampton
- Donald M. Hassler
- E. E. DeLuca
- E. K. Sutton
- E. Spanswick
- Emily Mason
- Erika Palmerio
- Go Murakami
- H. Cremades
- Hyomin Kim
- J. Benkhoff
- J. G. Luhmann
- J. P. Thayer
- J. T. Hoeksema
- J. Zhang
- James Turtle
- Jeffrey Newmark
- Jia Huang
- Jia Yue
- K. E. Korreck
- K. Hosokawa
- K. W. Paulson
- Katherine Garcia‐Sage
- Kazushi Asamura
- L. A. Balmaceda
- L. Golub
- L. K. Jian
- L. P. Chitta
- L. Rastäetter
- Lisa Upton
- M. L. Mays
- M. Lessard
- M. Nosé
- Manuela Temmer
- Marc L. DeRosa
- Maria D. Kazachenko
- Martin A. Reiss
- Masaaki Teramoto
- Mateja Dumbović
- Matthew A. Young
- Matthew J. West
- Md Nazmus Sakib
- Miki Kawamura
- N. A. Murphy
- N. A. Schwadron
- N. E. Raouafi
- N. M. Viall
- N. V. Pogorelov
- Nicolas André
- Nikolaos Paschalidis
- Nishu Karna
- P. Gonçalves
- Pete Riley
- Petrus C. Martens
- Phillip Hess
- R. D’Amicis
- R. H. Varney
- Raphaël Attié
- Rebecca Ringuette
- Reiko Nomura
- Riley Troyer
- Ronald M. Caplan
- Ryan McGranaghan
- S. D. Bale
- S. E. Gibson
- S. I. Jones
- S. Parenti
- S. T. Lepri
- S. Tomczyk
- Sabrina Savage
- Sarah A. Kovac
- Shadia Rifai Habbal
- Silvina Guidoni
- T. Dudok de Wit
- T. K. Kim
- Takeshi Sakanoi
- Taku Namekawa
- Talwinder Singh
- Tatiana Niembro
- V. Ledvina
- V. S. Titov
- W. D. Pesnell
- Xudong Sun
- Y. Ogawa
- Yeimy Rivera
- Yoshizumi Miyoshi