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Over the last decades, big effort has been carried out for characterization of plasmas found in galactic medium. The general purpose of this fourth book is to display a very complete set of plasma properties of sun and solar-like stars computed with the developed code ATMED CR (ATom MEDium Collisional Radiative). The graphical and tabulated results of plasmas also computed in the previous books (ISBN's 978-620-2-01943-9, 978-613-9-94744-7 & 978-620-0-31273-0) focus the attention on the order of magnitude of main parameters as mean charge, matter density, temperatures and rates. It also…mehr

Produktbeschreibung
Over the last decades, big effort has been carried out for characterization of plasmas found in galactic medium. The general purpose of this fourth book is to display a very complete set of plasma properties of sun and solar-like stars computed with the developed code ATMED CR (ATom MEDium Collisional Radiative). The graphical and tabulated results of plasmas also computed in the previous books (ISBN's 978-620-2-01943-9, 978-613-9-94744-7 & 978-620-0-31273-0) focus the attention on the order of magnitude of main parameters as mean charge, matter density, temperatures and rates. It also includes data of plasmas belonging to the NLTE-11 Workshop database, highlighting specifically results of thick plasmas and with injection of hot electrons for which using multiplier coefficients in plasma parameters gives way to random errors and must be totally forbidden.
Autorenporträt
Industrial Engineer. Master of Nuclear Science and Technology. PhD in Plasma and Atomic Physics. ETSII UPM (Oct. 2010 ¿ Sept. 2017): Master & Doctoral Thesis Elaboration: Collisional Radiative Average Atom Code Based on a Relativistic Screened Hydrogenic Atomic Model. ENERGY SECTOR (August 1999 ¿ Sept. 2009): Project Engineer for Power Plants.