Ionization Equation
Meghnad Saha formulates the thermal ionization equation that links stellar temperatures with the ionization states seen in spectra.
Follow Meghnad Saha through 2 dated historical records for India.
A chronological timeline drawn from matching World History Database records.
Meghnad Saha formulates the thermal ionization equation that links stellar temperatures with the ionization states seen in spectra.
Saha applies ionization theory to explain changes in stellar spectral lines as functions of temperature and pressure.
These dates and descriptions come from the historical_events database. Exact duplicate records have been collapsed. Names are grouped by the country, Name 2 and Name 1 fields; records with missing Name 2 cannot be reliably assigned to an individual biography. Check the underlying sources before formal citation.