Barkla characteristic X-ray experiment 2026-10-18
Charles Glover Barkla's 1911 paper describes irradiating a target with an X-ray tube and observing secondary X-rays using an electroscope. For soft Characteristic X-rays from tin, he used a soft primary beam and placed the electroscope close to the target to limit loss in air. Successive aluminium absorbers changed the gas-ionization signal. Thick absorbers suppressed the soft component; a carbon radiator supplied a comparison for the surviving scattered component. Subtracting this estimated contribution left approximately equal fractional losses through successive sheets, evidence for a nearly homogeneous component. Changing primary-beam hardness could suppress excitation of the more penetrating characteristic component.[ref]
The Spectra of the Fluorescent Röntgen Radiations by Charles Glover Barkla. Barkla, The spectra of the fluorescent Röntgen radiations (1911), p. 396: soft tube, nearby electroscope, aluminium sheets, carbon comparison and subtraction
An electroscope reads loss of stored electric charge; ionization in its detecting gas enables discharge. An ionization chamber with an electrometer instead measures the collected electric charge or electric current. These are integrating readouts: neither directly assigns an energy to each arriving photon. The diagram separates these functions without claiming a surviving apparatus drawing.
The K and L components were distinguished by their penetrating power and dependence on the emitting chemical element. Barkla's Nobel lecture, delivered on 3 June 1920 for the 1917 prize, explains that absorber-defined K radiation had seemed homogeneous, whereas later diffraction experiments resolved neighbouring spectral lines in both K and L groups. Absorber tests therefore distinguished groups without resolving every line.[ref]
Characteristic Röntgen Radiation by Charles Glover Barkla. Nobel Lectures, Physics 1901–1921; Barkla, Characteristic Röntgen radiation, printed pp. 392 and 395, PDF pp. 132 and 135: lecture date and limitations of absorption analysis
Henry Gwyn Jeffreys Moseley subsequently related the frequencies of corresponding spectral lines to atomic number. The approximate relation , with series-dependent constants , is Moseley's law; its discovery should be distinguished from Barkla's identification of characteristic secondary radiation.[ref]
Moseley and X Rays by University of Oxford Department of Physics. University of Oxford Department of Physics, Moseley and X rays: Moseley's graph and the story of Moseley and X-rays
A continuous incident frequency spectrum can contribute a continuous scattered background alongside discrete Characteristic X-rays. Here “scattered” identifies a production process, not a universal spectral shape: scattering of a narrow incident line need not make a continuum. In particular, the characteristic component is photon emission after vacancy creation, rather than simply the primary beam redirected. Source hardness, target substitution and absorber thickness probe different parts of that distinction. A surviving signal alone establishes neither an additional electron shell nor a fully resolved spectral line.
Nobel Lectures, Physics 1901–1921 Characteristic Röntgen Radiation by Charles Glover Barkla 2026-10-18
By Charles Glover Barkla. Nobel lecture delivered 3 June 1920, associated with the 1917 prize; award, lecture and upload years differ.
Nobel Prize in Physics in 1917 2026-10-18
Awarded to Charles Glover Barkla for characteristic X-rays of the chemical elements; he received it in 1918. The Barkla characteristic X-ray experiment describes the experimental separation of components.[ref]
The Nobel Prize in Physics 1917 by Nobel Prize Outreach. Official award record: Barkla, characteristic radiation and deferred receipt in 1918
By Charles Glover Barkla. Philosophical Magazine, series 6, 22, 396–412 (1911). Zenodo hosts the original article reproduction.
