HelioWebJ. A. Klimchuk
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A[J. A. Klimchuk]
AC["Associated Concepts (24)"]
AW["Authored Works (39)"]
CA["Linked Co-Authors (10)"]
CI["Linked Collaborating Institutions (43)"]
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AW== author ==>CA
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click AW "#authored-works"
click CA "#co-authors"
click CI "#collaborating-institutions"
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- ORCiD
- https://orcid.org/0000-0003-2255-0305
- OpenAlex ID
- https://openalex.org/A5049141219 (API record)
Associated Concepts [?]
- Physics
- Quantum mechanics
- Magnetic field
- Nuclear physics
- Astrophysics
- Plasma
- Biology
- Astronomy
- Solar wind
- Coronal mass ejection
- Astrobiology
- Mathematics
- Geography
- Venus
- Corona (planetary geology)
- Materials science
- Coronal loop
- Engineering
- Computer science
- Optics
- Thermodynamics
- Geology
- Nanoflares
- Meteorology
Authored Works
sorted by decreasing year, and then by display-name
- The Role of 3D Complexity in Magnetic Reconnection
- Implication of line tied magnetic field on magnetic reconnection in the closed corona
- Study of Type III Radio bursts in the Closed Corona and the Solar Wind from Small-scale Reconnection: Observations
- Onset of Magnetic Reconnection in the Solar Corona
- Magnetic Reconnection in 3D vs. 2D and Dependence on Magnetic Shear
- Distributed Space Telescopes Enabled by Constellation of Small Satellites
- Coronal Heating: A Coupled Multi-Scale Problem
- Computing Emission Signatures from Coronal MHD Models Without a Realistic Lower Atmosphere
- The Onset of Magnetic Reconnection
- The Details of Coronal Heating Matter!
- Reconnection Between Twisted Flux Tubes - Implications for Coronal Heating
- Nanoflare Heating of the Quiet Sun
- Hard X-ray Detectability of Small Impulsive Heating Events in the Solar Corona
- Capabilities of a FOXSI Small Explorer
- The Onset of Magnetic Reconnection in the Solar Atmosphere
- Intensity Conserving Spline Interpolation (ICSI): A New Tool for Spectroscopic Analysis
- Hi-C Observations and the Structure of Coronal Loops
- Space Physics and Aeronomy Section Agency NIght
- Line Profile Asymmetries, Densities, Spicules, and Nanoflares
- Coronal Heating Diagnostics from EUNIS 2013
- A Survey of Nanoflare Properties in Solar Active Regions
- The Role of Type II Spicules in the Upper Solar Atmosphere
- Nanoflare Heating of the Solar Corona: Comparing SDO/AIA Observations with Modeled Light Curves
- Exploring Small Spatial Scales in the Transition Region and Solar Corona with the Very High Angular Resolution Imaging Spectrometer (VERIS)
- Diagnosing the Time-Dependence of Active Region Core Heating Using Emission Measures
- Understanding Coronal Heating with Emission Measure Distributions
- Determining the Typical Nanoflare Cadence in Active Regions: Modeling Light Curves of Active Regions
- SDO/AIA Light Curves and Implications for Coronal Heating: Observations
- SDO/AIA Light Curves and Implications for Coronal Heating: Model Predictions
- Modeling the Secondary Flare Irradiance Measured by Solar Dynamic Observatory (SDO) Extreme ultraviolet Variability Experiment (EVE)
- The Existence and Origin of Turbulence in Solar Active Regions
- Understanding Warm Coronal Loops
- Explosive Instability and Coronal Heating
- Why We Need Imaging Spectroscopy
- Observing the Solar atmosphere with the Extreme Ultraviolet Imaging Spectrometer on Solar B
- Coronal Seismology and the Propagation of Acoustic Waves Along Coronal Loops
- The Non-flare Emisson Measure Above 5 MK Observed By RHESSI and SXI
- Linear Force Free Field Models of Observed Coronal Loops
- Bright Knots in EUV Post-flare Loops : TRACE Observations and 1D Hydrodynamic Modeling
Linked Co-Authors
- B. R. Dennis
- D. M. Rabin
- Durgesh Tripathi
- J. E. Leake
- J. G. Sample
- Jeffrey W. Reep
- L. K. S. Daldorff
- Natasha L. S. Jeffrey
- Steven Christe
- V. M. Uritsky
Linked Collaborating Institutions
- ADNET Systems Inc., Greenbelt, Maryland
- Artep, Inc., Washington, DC
- California Institute of Technology
- Catholic University, Washington DC
- E.O. Hulburt Center for Space Research, NRL
- George Mason University, Virginia
- Georgia Institute of Technology
- Goddard Space Flight Center, Astrophysics Division
- Inter-University Centre for Astronomy and Astrophysics, India
- Johns Hopkins University, Maryland
- KTH, Royal Institute of Technology, Sweden
- Kirtland Air Force Research Laboratory, New Mexico
- Montana State University, Bozeman
- NASA Goddard Space Flight Center, Maryland
- NASA Marshall Space Flight Center
- National Science Foundation
- New Jersey Institute of Technology
- New Mexico State University
- Purdue University, Indiana
- Rice University, Department of Physics and Astronomy
- Royal Observatory of Belgium
- Rutherford Appleton Laboratory
- Saint Andrews University, School of Mathematics and Statistics
- Southwest Research Institute, Boulder
- Stanford University, California
- The Ohio State University
- U.S. Department of the Navy, Naval Research Laboratory, Washington DC
- University of Calabria, Italy
- University of California, Berkeley
- University of California, Berkeley, Space Sciences Laboratory
- University of California, San Diego
- University of California, Santa Cruz
- University of Cambridge, Department of Applied Mathematics and Theoretical Physics
- University of Colorado, Boulder
- University of Colorado, Boulder, Laboratory for Atmospheric and Space Physics
- University of Glasgow, UK
- University of Illinois, Urbana-Champaign
- University of Ioannina, Department of Physics
- University of Ioannina, Greece
- University of Maryland, College Park
- University of Michigan
- University of Michigan, Department of Atmospheric Oceanic and Space Sciences
- Washington State University
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