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  2. Anode ray - Wikipedia

    en.wikipedia.org/wiki/Anode_ray

    These collide with atoms of the gas, knocking electrons off them and creating more positive ions. These ions and electrons in turn strike more atoms, creating more positive ions in a chain reaction. The positive ions are all attracted to the negative cathode, and some pass through the holes in the cathode. These are the anode rays.

  3. Electron - Wikipedia

    en.wikipedia.org/wiki/Electron

    The strongest bonds are formed by the sharing or transfer of electrons between atoms, allowing the formation of molecules. [17] Within a molecule, electrons move under the influence of several nuclei, and occupy molecular orbitals ; much as they can occupy atomic orbitals in isolated atoms. [ 128 ]

  4. Photoionization - Wikipedia

    en.wikipedia.org/wiki/Photoionization

    When either the laser intensity is further increased or a longer wavelength is applied as compared with the regime in which multi-photon ionization takes place, a quasi-stationary approach can be used and results in the distortion of the atomic potential in such a way that only a relatively low and narrow barrier between a bound state and the continuum states remains.

  5. Ives–Stilwell experiment - Wikipedia

    en.wikipedia.org/wiki/Ives–Stilwell_experiment

    These ions, after being accelerated to high speed in the canal ray tube, would interact with molecules of the fill gas (which sometimes included other gases than H 2) to release excited atomic hydrogen atoms whose velocities were determined by the charge-to-mass ratios of the parent H 2 + and H 3 + ions. [12]

  6. Cosmic ray spallation - Wikipedia

    en.wikipedia.org/wiki/Cosmic_ray_spallation

    Cosmic rays are highly energetic charged particles from beyond Earth, ranging from protons, alpha particles, and nuclei of many heavier elements. About 1% of cosmic rays also consist of free electrons. [citation needed] Cosmic rays cause spallation when a ray particle (e.g. a proton) impacts with matter, including other

  7. Photodissociation - Wikipedia

    en.wikipedia.org/wiki/Photodissociation

    The electrons reach the P700 reaction center of photosystem I where they are energized again by light. They are passed down another electron transport chain and finally combine with the coenzyme NADP + and protons outside the thylakoids to form NADPH. Thus, the net oxidation reaction of water photolysis can be written as:

  8. Cosmic ray - Wikipedia

    en.wikipedia.org/wiki/Cosmic_ray

    This abundance difference is a result of the way in which secondary cosmic rays are formed. Carbon and oxygen nuclei collide with interstellar matter to form lithium, beryllium, and boron, an example of cosmic ray spallation.

  9. Eugen Goldstein - Wikipedia

    en.wikipedia.org/wiki/Eugen_Goldstein

    Eugen Goldstein (/ ˈ ɔɪ ɡ ən / OY-gən, German: [ˈɔʏɡeːn ˈɡɔlt.ʃtaɪn, ˈɔʏɡn̩-]; 5 September 1850 – 25 December 1930) was a German physicist.He was an early investigator of discharge tubes, the discoverer of anode rays or canal rays, later identified as positive ions in the gas phase including the hydrogen ion.