JK
Member Since 1990
Jim A. Klimchuk
Research Astrophysicist, NASA Goddard Space Flight Center
AGU Research
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The Onset of Magnetic Reconnection in Thinning Current Sheets
FUNDAMENTAL PHYSICS OF THE SOLAR CORONA AND INNER HELIOSPHERE IV POSTER
spa-solar and heliospheric physics | 15 december 2023
James A. Klimchuk, James E. Leake, Lars K. Daldorf...
Many phenomena in the heliosphere and throughout the universe involve the explosive release of magnetic energy via fast reconnection at current sheets...
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Implication of line tied magnetic field on magnetic reconnection in the closed corona
FUNDAMENTAL PHYSICS OF THE SOLAR CORONA AND INNER HELIOSPHERE II ORAL
spa-solar and heliospheric physics | 13 december 2023
Lars K. Daldorff, James E. Leake, James A. Klimchu...
Magnetic reconnection plays an important role in the rapid release ofstored magnetic energy in the solar corona. This includes small eventslike nanofl...
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Nanoflare Statistics in a Driven Magnetically Closed Corona
SOLAR CORONAL HEATING: THEORY, OBSERVATIONS, AND SIMULATIONS I ELIGHTNING
spa-solar and heliospheric physics | 12 december 2023
Shanwlee Sow Mondal, Lars K. Daldorff, James A. Kl...
The complex granular motion of the solar photosphere serves as the primary source of energy to maintain the high temperature of magnetically closed co...
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Self-Consistent Heating of the Magnetically Closed Corona: Generation of Nanoflares and Response of the Plasma
SOLAR CORONAL HEATING: THEORY, OBSERVATIONS, AND SIMULATIONS I ELIGHTNING
spa-solar and heliospheric physics | 12 december 2023
Craig Johnston, Lars K. Daldorff, James A. Klimchu...
The energy that heats the magnetically closed solar corona originates in the complex motions of the massive photosphere. Turbulent photospheric convec...
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The Thickness of Current Sheets and Implications for Coronal Heating
SOLAR CORONAL HEATING: THEORY, OBSERVATIONS, AND SIMULATIONS I ELIGHTNING
spa-solar and heliospheric physics | 12 december 2023
James A. Klimchuk, James E. Leake, Lars K. Daldorf...
The thickness of current sheets is extremely important, especially as it relates to the onset of fast magnetic reconnection. Onset determines how much...
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The CubeSat Imaging X-ray Solar Spectrometer (CubIXSS): a new mission to understand heating of coronal plasma
SOLAR CORONAL HEATING: THEORY, OBSERVATIONS, AND SIMULATIONS II POSTER
spa-solar and heliospheric physics | 12 december 2023
Amir Caspi, P. S. Athiray, Will Barnes, Chun Ming ...
The CubeSat Imaging X-ray Solar Spectrometer (CubIXSS) is a 16U CubeSat funded under NASA H-FORT. CubIXSS is motivated by a compelling overarching sci...
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Implication of line tied magnetic field on magnetic reconnection in the closed corona
FUNDAMENTAL PHYSICS OF THE SOLAR CORONA AND INNER HELIOSPHERE IV ORAL
spa-solar and heliospheric physics | 15 december 2022
Lars K. Daldorff, James E. Leake, James A. Klimchu...
Magnetic reconnection plays an important role in heating the solar coronal plasma, as well as in the rapid release of magnetic energy stored in the co...
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The Role of 3D Complexity in Magnetic Reconnection
TURBULENCE, MAGNETIC RECONNECTION, AND PARTICLE ENERGIZATION THROUGHOUT HELIOSPHERE I ORAL
spa-solar and heliospheric physics | 12 december 2022
James A. Klimchuk, Lars K. Daldorff, James E. Leak...
Three-dimensional effects related to the presence of a guide field component can have a major impact on magnetic reconnection. They can allow reconnec...
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