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  2. Hydrogen line - Wikipedia

    en.wikipedia.org/wiki/Hydrogen_line

    A hydrogen atom with proton and electron spins aligned (top) undergoes a flip of the electron spin, resulting in emission of a photon with a 21 cm wavelength (bottom) The hydrogen line, 21 centimeter line, or H I line [a] is a spectral line that is created by a change in the energy state of solitary, electrically neutral hydrogen atoms.

  3. Intensity mapping - Wikipedia

    en.wikipedia.org/wiki/Intensity_mapping

    Detecting the 21 cm emission from this time, all the way through to the end of reionization, has been proposed as a powerful way of studying early structure formation. [9] This period of the Universe's history corresponds to redshifts of z ≈ 30 {\displaystyle z\approx 30} to z ≈ 6 − 12 {\displaystyle z\approx 6-12} , implying a frequency ...

  4. Primeval Structure Telescope - Wikipedia

    en.wikipedia.org/wiki/Primeval_Structure_Telescope

    The hydrogen line, 21 centimeter line or HI line refers to the electromagnetic radiation spectral line that is created by a change in the energy state of neutral hydrogen atoms. This electromagnetic radiation is at the precise frequency of 1420.40575177 MHz, which is equivalent to the vacuum wavelength of 21.10611405413 cm in free space.

  5. Water hole (radio) - Wikipedia

    en.wikipedia.org/wiki/Water_hole_(radio)

    The waterhole, or water hole, is an especially quiet band of the electromagnetic spectrum between 1420 and 1662 megahertz, corresponding to wavelengths of 18–21 centimeters. It is a popular observing frequency used by radio telescopes in radio astronomy. [1]

  6. Hydrogen spectral series - Wikipedia

    en.wikipedia.org/wiki/Hydrogen_spectral_series

    For example, the 2 → 1 line is called "Lyman-alpha" (Ly-α), while the 7 → 3 line is called "Paschen-delta" (Pa-δ). Energy level diagram of electrons in hydrogen atom. There are emission lines from hydrogen that fall outside of these series, such as the 21 cm line.

  7. Hydrogen maser - Wikipedia

    en.wikipedia.org/wiki/Hydrogen_maser

    The amount of energy needed to reverse the spin of the electron is equivalent to a photon at the frequency of 1.420 405 751 768 GHz, [1] which corresponds to the 21 cm line in the hydrogen spectrum. Hydrogen masers are very complex devices and sell for as much as US$235,000. [2] There are two types to be distinguished: active and passive.

  8. Hyperfine structure - Wikipedia

    en.wikipedia.org/wiki/Hyperfine_structure

    Hyperfine structure gives the 21 cm line observed in H I regions in interstellar medium. Carl Sagan and Frank Drake considered the hyperfine transition of hydrogen to be a sufficiently universal phenomenon so as to be used as a base unit of time and length on the Pioneer plaque and later Voyager Golden Record.

  9. Hydrogen Intensity and Real-time Analysis eXperiment

    en.wikipedia.org/wiki/Hydrogen_Intensity_and...

    This is accomplished by looking at the 21-cm line emission produced by hot diffuse neutral hydrogen from distant galaxy clusters and from the intracluster medium. [1] This neutral hydrogen traces out the large scale structures in the universe, and so can be used to map out the large scale Baryon Acoustic Oscillation (BAO) structure of the universe.

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