Juan M. Fontenla NorthWest Research Associates (NWRA) Boulder, CO [email protected] Juan M. Fontenla received his Ph. D. in Physics from the University of Buenos Aires, Argentina, in 1986. His thesis introduced a new a numerical algorithm for computing transport coefficients in partially ionized complex astrophysical plasmas. During his undergraduate studies he worked at the Observatory of San Miguel, Argentina, on solar instrumentation and observational research, developed a non-LTE radiative transfer algorithm, and its code for modeling prominences. In 1982, he joined the Institute for Astronomy and Space Physics (IAFE, Argentina) performing observational work on stellar objects and theoretical research in Solar Physics and Astrophysics. He gave courses at the Observatory of La Plata in Argentina, and codirected students at the University of Buenos Aires. In 1986, Dr. Fontenla was awarded an NRC-Research Associateship at the Marshall Space Flight Center (MSFC, Huntsville, Alabama) for working on UVSP/Solar Max Mission data with Dr. Tandberg-Hanssen. This research at MSFC produced a number of papers on solar Lyα emission, microflares and flares in UV and X-rays and prominence eruption. In 1989 he moved to the University of Alabama in Huntsville for studying MSFC vector magnetic field observations related to flares, continuing studies on UVSP data, and applying particle diffusion and energy balance to solar transition region atmospheric non-LTE models in collaboration with Dr. Avrett. In 1994, Dr. Fontenla moved to the High Altitude Observatory (Boulder, CO) for work on the solar irradiance synthesis project lead by Dr. White. In the period 1996-2002, Dr. Fontenla worked in private software companies, including commercial, IT, and medical, and lead software development. During this time, Dr. Fontenla continued his collaborations with Drs. White and Avrett, and developed a new and extensive C++ code library, the Solar Radiation Physical Modeling (SRPM) system, for solving the non-LTE radiative transfer and computing the solar irradiance spectrum in all its details. In 2002 Dr. Fontenla joined the Laboratory for Aeronomy and Space Physics (LASP, Boulder, CO), working on algorithms for processing data from the SORCE satellite. In 2013, Dr. Fontenla moved to NorthWest Research Associates (in Boulder, CO) where he currently works on applications of SRPM computations of the variations in solar spectral irradiance, driven by observations of the Sun, to middle and upper Earth atmosphere modeling. He also studies other topics relevant to weakly-and fully-ionized plasma behavior and energy balance in solar, stellar, and planetary atmospheres. Dr. Fontenla is a member of the American Geophysical Union, the American Astronomical Society, and the International Astronomical Union. 0
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