Ross Galbreath 2026-10-18
CERN 2026-10-18
Institutional issuer of Cosmic Rays: Particles from Outer Space by CERN.
C. Arcaro b. Schultz 2026-10-18
Credit retained as printed.
Tekniska museet 2026-10-18
Institutional museum source issuer.
C. R. Mann Created 2026-10-18 Updated 2026-11-05
A physics educator whose 1912 book addressed the organization and purpose of physics teaching. In the author’s preface he rejected a rigid sequence of prescribed lessons: a teacher must think independently and adapt the work to the local setting. The book documents an attempt to make instruction in physics serve active scientific reasoning rather than depend on a universal classroom recipe.[ref]
The Teaching of Physics for Purposes of General Education by C. R. Mann. Title page and Author’s Preface, pp. vii–ix
J. Chang Created 2026-10-18 Updated 2026-11-05
A contributor to the NIST charged-particle stopping and range databases. Their energy-dependent tables make calculated electron stopping power and ion energy losses reusable across materials. The tabulated ranges summarize slowing behavior while keeping the particle type and initial energy explicit.[ref]
Stopping-Power and Range Tables for Electrons, Protons, and Helium Ions by M. J. Berger and others. Database credit and ESTAR/PSTAR/ASTAR descriptions
M. A. Zucker Created 2026-10-18 Updated 2026-11-05
A researcher whose joint reference-data work provides charged-particle stopping power and continuous slowing-down approximation range. Integrating the inverse energy-loss rate estimates a path length, giving users a consistent way to connect local energy loss with an overall slowing distance.[ref]
Stopping-Power and Range Tables for Electrons, Protons, and Helium Ions by M. J. Berger and others. Introduction and range definitions: stopping-power integration and CSDA range
J. S. Coursey Created 2026-10-18 Updated 2026-11-05
M. J. Berger Created 2026-10-18 Updated 2026-11-05
A researcher whose joint NIST reference work tabulates stopping power and particle ranges. These quantities describe how charged particles lose energy in matter and how far they travel while slowing. The tables turn microscopic interaction calculations into inputs for detector and radiation-transport estimates.[ref]
Stopping-Power and Range Tables for Electrons, Protons, and Helium Ions by M. J. Berger and others. Introduction and ESTAR/PSTAR/ASTAR descriptions: calculated energy losses and ranges
Massachusetts Institute of Technology, Technical Services Group Created 2026-10-18 Updated 2026-11-05
S. Edyvean Created 2026-10-18 Updated 2026-11-05
A scientific teaching contributor credited with the initial work used for an IAEA slide set on X-ray production. The shared material explains how tube operating conditions and filtration change the radiation output, helping distinguish the amount of radiation from the distribution of photon energies.[ref]
R. Nowotny Created 2026-10-18 Updated 2026-11-05
A scientific author credited with the chapter underlying the IAEA teaching slides on X-ray production. The treatment links electron acceleration, target interactions and tube design with the emitted X-ray spectrum. This connects the physical origin of radiation with the practical variables used to control a laboratory or diagnostic source.[ref]
K. P. Maher Created 2026-10-18 Updated 2026-11-05
A scientific teaching contributor credited with preparing the IAEA slide set on X-ray production. The material distinguishes continuous bremsstrahlung from discrete Characteristic X-rays and relates both to the operation of an X-ray tube. That distinction helps students interpret a tube’s output spectrum in terms of different physical mechanisms.[ref]
Chapter 5: X-Ray Production (teaching slides) by K. P. Maher. Title slide: slide-preparation credit; §§5.2–5.3: production mechanisms and tube components
Jean E. Sansonetti Created 2026-10-18 Updated 2026-11-05
A spectroscopic-data researcher whose joint NIST handbook organizes spectral lines, atomic energy levels and transition probabilities. These linked tables let an observer connect a measured wavelength with possible atomic transitions. Recording the energy-level classification alongside a line makes the database useful for interpreting a spectrum, beyond simply listing bright wavelengths.[ref]
Handbook of Basic Atomic Spectroscopic Data by Jean E. Sansonetti and William C. Martin. Database authors; Strong-Line, Persistent-Line and Energy-Level Tables
Arthur Stanton 2026-10-18
Susanne Kiewitz 2026-10-18
Lorenz Friedrich Beck 2026-10-18
J. Zhang Created 2026-10-18 Updated 2026-11-05
A researcher whose joint work measured the Brownian motion of an ellipsoid using both a laboratory frame and a frame that rotates with the particle. The two descriptions expose different displacement statistics. This provides an experimental example of why a random trajectory must be analyzed with its changing orientation, rather than position alone.[ref]
Brownian Motion of an Ellipsoid by Yilong Han and others. pp. 626–628, Figs. 1–3: coordinate frames and displacement distributions
M. Nobili Created 2026-10-18 Updated 2026-11-05
A researcher whose team investigated the coupling of rotational diffusion and translational diffusion in a freely moving ellipsoid. At short times the particle remembers its orientation, while at longer times rotation averages over directions. The experiment shows how the timescale of observation changes the apparent symmetry of Brownian motion.[ref]
Brownian Motion of an Ellipsoid by Yilong Han and others. pp. 627–628, Figs. 2–3: rotational relaxation and laboratory-frame motion
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