HelioWebR. A. Frazin
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A[R. A. Frazin]
AC["Associated Concepts (25)"]
AW["Authored Works (42)"]
CA["Linked Co-Authors (7)"]
CI["Linked Collaborating Institutions (29)"]
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AW== author ==>CA
AW== affil ==>CI
click AC "#associated-concepts"
click AW "#authored-works"
click CA "#co-authors"
click CI "#collaborating-institutions"
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- ORCiD
- https://orcid.org/0000-0002-0281-7677
- OpenAlex ID
- https://openalex.org/A5079674409 (API record)
Associated Concepts [?]
- Physics
- Quantum mechanics
- Astronomy
- Optics
- Computer science
- Biology
- Astrophysics
- Astrobiology
- Computer vision
- Nuclear physics
- Geology
- Plasma
- Geography
- Venus
- Magnetic field
- Corona (planetary geology)
- Solar wind
- Mathematics
- Artificial intelligence
- Medicine
- Stars
- Coronal mass ejection
- Radiology
- Engineering
- Planet
Authored Works
sorted by decreasing year, and then by display-name
- Three-Dimensional Tomographic Reconstruction and MHD Modeling of the Solar Corona and Wind: WHPI Campaign Rotations CR-2219 and CR-2223
- Metis - Solar Orbiter Topical Team on "Modelling of CME propagation/evolution in corona and solar wind in connection with Space Weather"
- Tomographic Validation of the AWSoM Model of the Inner Corona During Solar Minima
- Solar Minima Comparative Analysis Using EUV Tomography
- Energy Balance in Magnetic Loops of the Quiet Sun
- Ensemble Space Weather Forecasting with the SWMF
- Coronal Hole Boundaries as Source Regions of a Steady Slow Solar Wind: Global Modeling of Charge State Composition and Sun-to-Earth Observations
- The Multi-thermal Plasma of Coronal Streamers as seen with SDO/AIA Tomography
- One-Hour Cadence Comparison of the AWSoM 3D MHD Model to LASCO-C2
- Inverted Temperature Loops in The Quiet Corona: Properties and Physical Origin
- Understanding Inverted Temperature Loops in the Quiet Sun Corona With 3D, Global MHD Modeling
- Testing a Two-temperature Model of the Solar Corona with Empirically-derived Plasma parameters
- Evolution of the Global Temperature Structure of the Solar Corona Around the Last Solar Minimum
- CME Reconstruction from Three Viewpoints Via Simulation Morphing
- A Study of the Thermodynamical Properties of Streamers and Pseudo-Streamers
- The First EUVI Images Seen Without Stray Light
- Modeling Solar Wind and Coronal Mass Ejection During Carrington Rotation 2107
- Integrating Tomography and Global Simulation
- Global Temperature Structures Determined from DEMT
- EUV Tomography and Global Magnetic Modeling of the Solar Corona during the Solar Cycle 24 Rising Phase
- Testing Nonuniform Heating RTV-Type Models of Coronal Loops with 3D Differential Emission Measure Tomography
- Prominence Cavities from Differential Emission Measure Tomography
- Partition of Proton and Electron Heating in the Solar Wind (Invited)
- Numerical Simulation of Earth Directed CMEs with an Advanced Two-Temperature Coronal Model (Invited)
- Multispacecraft Validation of a Global Two-Temperature Corona and Inner Heliosphere Model (Invited)
- Improving the physics models in the Space Weather Modeling Framework
- Differential Emission Tomography of AIA Images
- Coronal Heating by Surface Alfven Wave Damping: Implementation in MHD Modeling and Connection to Observations
- Turbulent Alfven Waves as a Solar Wind Driver: Results from a new 4D model for the Solar Corona and Solar Wind
- Tomography with LASCO-C2 Total Brightness Images
- An Assimilative 3-D Model of Coronal Density from Multi-Spacecraft Observations
- 3D Differential Emission Measure of the 2008 Solar Minimum Corona with Dual-Spacecraft EUVI/STEREO Tomography
- First Results of 3D, Global EUV Tomography from the STEREO Mission: Solar Minimum Results
- 4D Model for MHD Wave Turbulence in the Solar Corona and Solar Wind
- Global, 4D Differential Emission Measure Analysis of EIT 17.1, 19.5 and 28.4 nm Images
- Assimilative 3D Models of Density and Temperature in the Solar Corona
- Time Dependent Tomography of the Solar Corona in Three Spatial Dimensions
- Increased Spatial Resolution in 3D Tomography of the Corona with High Cadence pB images from LASCO-C2
- 3D Coronal Temperatures from Tomographic Analysis of EIT 17.1, 19.5 and 28.4 nm Images
- Time-Dependent Tomography of the Non-Stationary Corona with Multi-Spacecraft Image Data
- Response of the Electron Density in the Solar Corona to Extreme Solar Events
- On the use of STEREO Measurements for Solar Rotational Tomography
Linked Co-Authors
Linked Collaborating Institutions
- Academy of Sciences of the Czech Republic, Astronomical Institute
- Aix-Marseille Universite, Laboratoire d'Astrophysique
- CAS, Purple Mountain Observatory
- George Mason University, Virginia
- Indian Institute of Science Education and Research, Calcutta, India
- Institut d'Astrophysique Spatiale
- Italian Space Agency
- Los Alamos National Laboratory, New Mexico
- NASA Goddard Space Flight Center, Maryland
- NASA Marshall Space Flight Center
- RAL, Space Science and Technology Department
- Romanian Academy of Sciences
- Royal Observatory of Belgium
- Royal Observatory of Belgium, Department of Solar Physics
- Saint Andrews University, School of Mathematics and Statistics
- Tor Vergata University, Rome, Italy
- University College London, Mullard Space Science Laboratory
- University of Buenos Aires, Argentina
- University of Florence, Italy
- University of Hawaii, Manoa, Institute for Astronomy
- University of Helsinki, Finland
- University of Illinois, Urbana-Champaign
- University of L'Aquila, Italy
- University of Michigan
- University of Michigan, Department of Atmospheric Oceanic and Space Sciences
- University of Michigan, Space Physics Research Laboratory
- University of Palermo, Department of Physics
- University of Palermo, Italy
- University of Wroclaw, Poland
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