Gregory D. Fleishman

TL;DR: In this article, the first science results from the newly completed expanded Owens Valley solar array (EOVSA) were reported, which obtained excellent microwave imaging spectroscopy observations of SOL2017-09-10, a classic partially-occulted solar limb flare associated with an erupting flux rope.

TL;DR: In this article, the authors developed approximate gyrosynchrotron (GS) codes capable of quickly calculating the GS emission (in non-quantum regime) from both isotropic and anisotropic electron distributions in non-relativistic, mildly relativistic and ultrarelatio-ivistic energy domains applicable throughout a broad range of source parameters including dense or tenuous plasmas and weak or strong magnetic fields.

TL;DR: In this paper, numerical calculations of the intensity, degree of polarization, and spectral index of gyrosynchrotron emission produced by fast electrons with anisotropic pitch-angle distributions are presented.

TL;DR: In this paper, an enhanced software architecture allows the user to import photospheric magnetic field maps and perform magnetic field extrapolations to generate 3D magnetic field models; investigate the magnetic topology by interactively creating field lines and associated flux tubes; populate the flux tubes with user-defined non-uniform thermal plasma and anisotropic, nonuniform, non-thermal electron distributions; and compare the model-derived images and spectra with observational data.

TL;DR: The Atacama Large Millimeter/submillimeter Array (ALMA) as discussed by the authors is a powerful tool for observing the Sun at high spatial, temporal, and spectral resolution, which can address a broad range of fundamental scientific questions in solar physics.