MHD models predict that above 10 keV the solar magnetic field collimates plasma into high-latitude lobes, producing a factor of ~2 ENA enhancement at 80 keV that IMAP can detect.
2016 THE MYSTERIOUS CASE OF THE SOLAR ARGON ABUNDANCE NEAR SUNSPOTS IN FLARES
6 Pith papers cite this work. Polarity classification is still indexing.
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Sulphur abundances decrease above 150 G in coronal loops, indicating FIP fractionation is modulated by mean magnetic field strength.
Hybrid neutron star EOS constructed from DDME2 hadronic and two-flavor NJL quark models with quintic interpolation requires early crossover near saturation density to satisfy PSR J0740+6620 mass and NICER radius constraints.
Numerical and analytical modeling of cosmic-ray transport attributes the long-term variation in the AMS-observed proton-to-helium ratio below 3 GV to mass-to-charge dependence in the heliospheric diffusion coefficient.
The thesis assesses the reliability of stellar population synthesis modeling for galaxy physical properties using limited multi-band photometry rather than full spectra.
The review identifies and discusses key unsolved problems in planetary nebulae such as 3D morphology, multipolar origins, dust distribution, binarity, and the abundance discrepancy, along with suggested future directions.
citing papers explorer
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Study of Neutron Star Properties under the Two-Flavor Quark NJL Model
Hybrid neutron star EOS constructed from DDME2 hadronic and two-flavor NJL quark models with quintic interpolation requires early crossover near saturation density to satisfy PSR J0740+6620 mass and NICER radius constraints.
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Numerical modeling of cosmic-ray transport in the heliosphere and interpretation of the proton-to-helium ratio in Solar Cycle 24
Numerical and analytical modeling of cosmic-ray transport attributes the long-term variation in the AMS-observed proton-to-helium ratio below 3 GV to mass-to-charge dependence in the heliospheric diffusion coefficient.