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Meghnad Saha

Physicist; ionisation and stellar-atmosphere theorist

Photograph · Image credit

Who they are

Meghnad Saha applied atomic ionisation theory to problems in the solar and stellar atmosphere. His 1920 paper considers how atoms and their ions contribute to observed spectral lines. That theoretical foundation is relevant to Cecilia Payne’s later analysis of stellar atmospheres and the relationship between spectra, physical conditions and inferred composition.

He is an acknowledged theoretical predecessor in the Payne milestone.

Selected contributions

  • Authored a 1920 paper applying ionisation physics to the solar chromosphere.Source ↗
  • Provided ionisation-theory foundations used in the stellar-atmosphere work discussed by the timeline.Source ↗Source 2 ↗

Selected works

  • Academic paper · 1920

    Ionisation in the Solar Chromosphere

    Applies atomic ionisation arguments to the solar atmosphere, beginning with the behavior of calcium and related spectral lines. This is a primary entry point to the ionisation physics later used in stellar-atmosphere analysis.

    Linked scan comes from the 1969 Collected Scientific Papers; the original article is Philosophical Magazine, series VI, volume 40, starting p. 472.

    Reading scope & citation

    First scan page visually read; 1920 Philosophical Magazine metadata checked in the Saha Institute catalogue. Remaining derivation not audited.

In the timeline

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Biography sources & portrait credit

Portrait credit

Unknown photographer. Public domain (Commons file-specific copyright declaration). Via Wikimedia Commons.

Photograph. Cropped to 4:5, resized to 320 × 400 and converted to WebP.

Image source & identification ↗ · Public domain (Commons file-specific copyright declaration) ↗