HelioWebN. A. Murphy
flowchart
A[N. A. Murphy]
AC["Associated Concepts (20)"]
AW["Authored Works (22)"]
CA["Linked Co-Authors (11)"]
CI["Linked Collaborating Institutions (27)"]
A== dcterms:relation ==>AC
AW== author ==>A
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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NO["add outgoing edge"]
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click NO "#add-outgoing-edge"
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- ORCiD
- https://orcid.org/0000-0001-6628-8033
- OpenAlex ID
- https://openalex.org/A5060645832 (API record)
Associated Concepts [?]
- Physics
- Quantum mechanics
- Nuclear physics
- Plasma
- Magnetic field
- Astronomy
- Computer science
- Astrophysics
- Engineering
- Biology
- Magnetic reconnection
- Geography
- Geology
- Magnetohydrodynamics
- Operating system
- Mathematics
- Solar wind
- Astrobiology
- Programming language
- Current sheet
Authored Works
sorted by decreasing year, and then by display-name
- XRTpy: A Python package for the X-Ray Telescope on Hinode
- The IRIS UV Burst Survey: Final Statistical Results and Semi-empirical Modeling Efforts
- Revisiting the Bastille Day Coronal Mass Ejection: Learning About the Eruption Through 3D MHD Time-Dependent Ionization Modeling of Heavy Ions
- In-line Non-equilibrium Ionization Calculation Module with Kappa Distribution in MHD Simulations
- Developing an Executable Paper With the Python in Heliophysics Community
- Constraining the CME Core's Heating and Energy Budget with SOHO/UVCS
- PlasmaPy: A Community Python Package for Plasma Physics
- Thermal energy creation and transport and X-ray/EUV emission in a thermodynamic MHD CME simulation
- Plasma Heating During Coronal Mass Ejections
- Non-Equilibrium Ionization Modeling of Coronal Mass Ejections
- Twisting/Rolling Motions and Chirality in Filament Eruptions
- Asymmetric Magnetic Reconnection in Partially Ionized Chromospheric Plasmas
- Constraining Models Of The Solar Chromosphere Using An X2 Flare Observed By SDO/EVE
- Asymmetric Magnetic Reconnection in the Solar Atmosphere
- Asymmetric Magnetic Reconnection in the Solar Atmosphere
- Ionization and Emission Characteristics of the Current Sheet in a CME/flare Eruption Mode
- Magnetic Reconnection X-Line Retreat Associated with Dipolarization of the Earth's Magnetosphere
- Asymmetric Magnetic Reconnection in Coronal Mass Ejection Current Sheets
- Transition Region Luminosities of Solar Flares
- Competing X-lines During Magnetic Reconnection
- Candidate coronal mass ejection heating mechanisms
- Plasma Heating Rates for a Coronal Mass Ejection on 28 June 2000
Linked Co-Authors
- C. A. Madsen
- Colby Haggerty
- Cooper Downs
- J. T. Niehof
- Jonathan D. Slavin
- K. E. Korreck
- Rebecca Ringuette
- S. T. Lepri
- Shawn Polson
- Yeimy Rivera
- Yihua Zheng
Linked Collaborating Institutions
- ASML Holdings, Netherlands
- Boston College, Massachusetts
- CAS, Purple Mountain Observatory
- CAS, Yunnan Observatory
- Florida Institute of Technology, Department of Physics and Space Science
- Georgia State University
- Harvard University, Massachusetts
- Imperial College, Department of Physics
- JAXA, Institute of Space and Astronautical Science
- Johns Hopkins University, Maryland
- Los Alamos National Laboratory, New Mexico
- NASA Goddard Space Flight Center, Maryland
- Nagoya University, Solar Terrestrial Environment Laboratory
- Predictive Science Inc., California
- Royal Observatory of Belgium
- Smithsonian Astrophysical Observatory
- U.S. Department of the Navy, Naval Research Laboratory, Washington DC
- University of California, Berkeley, Space Sciences Laboratory
- University of California, Los Angeles, Institute of Geophysics and Planetary Physics
- University of Chicago
- University of Colorado, Boulder
- University of Colorado, Boulder, Laboratory for Atmospheric and Space Physics
- University of Delaware
- University of Michigan
- University of New Hampshire
- University of North Dakota, Department of Space Studies
- University of Sheffield, UK
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