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Meghnad Saha FRS (6 October 1893 – 16 February 1956) was an Indian astrophysicist who helped devise the theory of thermal ionisation. His Saha ionisation equation allowed astronomers to accurately relate the spectral classes of stars to their actual temperatures.
Meghnad Saha (6 de octubre de 1893 – 16 de febrero de 1956) fue un astrofísico de la India, [1] [2] famoso por su desarrollo de la ecuación de Saha, que permite describir las condiciones químicas y físicas en las estrellas.
5 de abr. de 2024 · Meghnad N. Saha (born Oct. 6, 1893, Seoratali, near Dacca, India—died Feb. 16, 1956, New Delhi) was an Indian astrophysicist noted for his development in 1920 of the thermal ionization equation, which, in the form perfected by the British astrophysicist Edward A. Milne, has remained fundamental in all work on stellar atmospheres.
1 de ago. de 2016 · Meghnad Saha (1893–1956) was an Indian physicist who did much of his work in the last decades of British colonial rule. In the 1920s he made important contributions to the theory of thermal ionization and its application to stellar spectra.
A biography of Meghnad Saha, the Indian physicist who developed the theory of thermal ionization and the Saha equations. The book covers his scientific achievements, his role in building scientific institutions, and his political activities in India.
Meghnad Saha (6 de octubre de 1893 – 16 de febrero de 1956) fue un astrofísico de la India, famoso por su desarrollo de la ecuación de Saha, que permite describir las condiciones químicas y físicas en las estrellas.
Meghnad Saha (1893–1955) set out his theory in a number of papers published in British journals during 1920–1921. The work was immediately recognized as laying the foundation of quantitative astrophysics. Saha showed that astronomical spectra of 161 https://doi.org/10.1017/S1743921319000267 Published online by Cambridge University Press
