Search Results - "Nita, Gelu M."
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Decay of the coronal magnetic field can release sufficient energy to power a solar flare
Published in Science (American Association for the Advancement of Science) (17-01-2020)“…Solar flares are powered by a rapid release of energy in the solar corona, thought to be produced by the decay of the coronal magnetic field strength. Direct…”
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Solar flare accelerates nearly all electrons in a large coronal volume
Published in Nature (London) (23-06-2022)“…Solar flares, driven by prompt release of free magnetic energy in the solar corona 1 , 2 , are known to accelerate a substantial portion (ten per cent or more)…”
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Microwave and Hard X-Ray Observations of the 2017 September 10 Solar Limb Flare
Published in The Astrophysical journal (10-08-2018)“…We report the first science results from the newly completed Expanded Owens Valley Solar Array (EOVSA), which obtained excellent microwave (MW) imaging…”
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Magnetic Reconnection during the Post-impulsive Phase of a Long-duration Solar Flare: Bidirectional Outflows as a Cause of Microwave and X-Ray Bursts
Published in The Astrophysical journal (01-09-2020)“…Magnetic reconnection plays a crucial role in powering solar flares, production of energetic particles, and plasma heating. However, where the magnetic…”
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Data-constrained 3D Modeling of a Solar Flare Evolution: Acceleration, Transport, Heating, and Energy Budget
Published in The Astrophysical journal (01-08-2023)“…Abstract Solar flares are driven by the release of free magnetic energy and its conversion to other forms of energy—kinetic, thermal, and nonthermal…”
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Measurement of magnetic field and relativistic electrons along a solar flare current sheet
Published in Nature astronomy (01-12-2020)“…In the standard model of solar flares, a large-scale reconnection current sheet is postulated to be the central engine for powering the flare energy release 1…”
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THREE-DIMENSIONAL RADIO AND X-RAY MODELING AND DATA ANALYSIS SOFTWARE: REVEALING FLARE COMPLEXITY
Published in The Astrophysical journal (01-02-2015)“…Many problems in solar physics require analysis of imaging data obtained in multiple wavelength domains with differing spatial resolution in a framework…”
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Three-dimensional Forward-fit Modeling of the Hard X-Ray and Microwave Emissions of the 2015 June 22 M6.5 Flare
Published in The Astrophysical journal (01-01-2018)“…The well-established notion of a "common population" of the accelerated electrons simultaneously producing the hard X-ray (HXR) and microwave (MW) emission…”
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Data-constrained Solar Modeling with GX Simulator
Published in The Astrophysical journal. Supplement series (01-07-2023)“…To facilitate the study of solarflares and active regions, we have created a modeling framework, the freelydistributed GX Simulator IDL package, that combines…”
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Time Series of Magnetic Field Parameters of Merged MDI and HMI Space-weather Active Region Patches as Potential Tool for Solar Flare Forecasting
Published in The Astrophysical journal (01-09-2024)“…Abstract Solar flare prediction studies have been recently conducted with the use of Space-Weather MDI (Michelson Doppler Imager on board Solar and…”
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Statistical Study of the Correlation between Solar Energetic Particles and Properties of Active Regions
Published in The Astrophysical journal (01-08-2023)“…Abstract The flux of energetic particles originating from the Sun fluctuates during the solar cycles. It depends on the number and properties of active regions…”
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Predicting Solar Proton Events of Solar Cycles 22–24 Using GOES Proton and Soft-X-Ray Flux Features
Published in The Astrophysical journal. Supplement series (01-01-2024)“…Abstract Solar energetic particle (SEP) events and their major subclass, solar proton events (SPEs), can have unfavorable consequences on numerous aspects of…”
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NARROWBAND GYROSYNCHROTRON BURSTS: PROBING ELECTRON ACCELERATION IN SOLAR FLARES
Published in The Astrophysical journal (20-07-2016)“…ABSTRACT Recently, in a few case studies we demonstrated that gyrosynchrotron microwave emission can be detected directly from the acceleration region when the…”
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Revealing the Evolution of Non-thermal Electrons in Solar Flares Using 3D Modeling
Published in The Astrophysical journal (20-05-2018)“…Understanding non-thermal particle generation, transport, and escape in solar flares requires detailed quantification of the particle evolution in the…”
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Radio Frequency Interference Excision Using Spectral‐Domain Statistics
Published in Publications of the Astronomical Society of the Pacific (01-07-2007)“…A radio frequency interference (RFI) excision algorithm based on spectral kurtosis, a spectral variant of time‐domain kurtosis, is proposed and implemented in…”
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Energy Budget of Plasma Motions, Heating, and Electron Acceleration in a Three-loop Solar Flare
Published in The Astrophysical journal (01-06-2021)“…Abstract Nonpotential magnetic energy promptly released in solar flares is converted to other forms of energy. This may include nonthermal energy of…”
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Understanding the Initiation of the M2.4 Flare on 2017 July 14
Published in The Astrophysical journal (01-12-2021)“…Abstract We present both the observation and the magnetohydrodynamics (MHD) simulation of the M2.4 flare (SOL2017-07-14T02:09) of NOAA active region (AR) 12665…”
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A Large-scale Plume in an X-class Solar Flare
Published in The Astrophysical journal (20-08-2017)“…Ever-increasing multi-frequency imaging of solar observations suggests that solar flares often involve more than one magnetic fluxtube. Some of the fluxtubes…”
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The Peak Flux Distribution of Solar Radio Bursts
Published in The Astrophysical journal (01-05-2002)Get full text
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Coronal Heating Law Constrained by Microwave Gyroresonant Emission
Published in The Astrophysical journal (01-03-2021)“…Abstract The question why the solar corona is much hotter than the visible solar surface still puzzles solar researchers. Most theories of the coronal heating…”
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