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  1. en.wikipedia.org › wiki › Meghnad_SahaMeghnad Saha - Wikipedia

    Meghnad Saha FRS [1] (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.

  2. c. 1934. Meghnad Saha FRS ( 6 de outubro de 1893 - 16 de fevereiro de 1956 [ 1]) foi um astrofísico indiano que desenvolveu a equação de ionização de Saha, usada para descrever as condições químicas e físicas das estrelas. [ 2][ 3] Seu trabalho permitiu aos astrônomos relacionar com precisão as classes espectrais de ...

  3. 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.

    • The Editors of Encyclopaedia Britannica
  4. 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.

  5. 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.

  6. Saha is justly regarded as one of the founders of theoretical astrophysics. Examination of his life and work is a rewarding exercise from various points of view: development of modern astronomy; Western science and the non-West; and political and social activism of a leading scientist and educator.

  7. Saha is justly regarded as one of the founders of theoretical astrophysics. Examination of his life and work is a rewarding exercise from various points of view: development of modern astronomy; Western science and the non-West; and political and social activism of a leading scientist and educator.