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This book helps the reader to understand influence of solar flares on the terrestrial conditions and different plasma properties of solar flares. The reader also gets an idea about ionization of heavy elements like Iron (Fe) and Molybdenum (Mo) and recombination processes, various rate coefficients and excitation processes of their ions in astrophysical plasma. Further the author has also determined and presented the fractional abundance, excitation rate coefficients and contribution functions of neutral atoms and ions and has proposed the possibility of population inversion and probability of…mehr

Produktbeschreibung
This book helps the reader to understand influence of solar flares on the terrestrial conditions and different plasma properties of solar flares. The reader also gets an idea about ionization of heavy elements like Iron (Fe) and Molybdenum (Mo) and recombination processes, various rate coefficients and excitation processes of their ions in astrophysical plasma. Further the author has also determined and presented the fractional abundance, excitation rate coefficients and contribution functions of neutral atoms and ions and has proposed the possibility of population inversion and probability of getting the stimulated emission from the astrophysical plasma.
Autorenporträt
The author is working as HoD of Electronics & I/C Principal, Yeshwant Mahavidyalaya, Nanded. He has 40 research papers to his credit & participated in more than 20 conferences at National/International Level & is working on Minor Research Project in Thin Film area. He has contributed to various bodies of SRTM University & recently visited Thailand.