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  2. Electron density - Wikipedia

    en.wikipedia.org/wiki/Electron_density

    Electron density or electronic density is the measure of the probability of an electron being present at an infinitesimal element of space surrounding any given point. It is a scalar quantity depending upon three spatial variables and is typically denoted as either ρ ( r ) {\displaystyle \rho ({\textbf {r}})} or n ( r ) {\displaystyle n ...

  3. Saha ionization equation - Wikipedia

    en.wikipedia.org/wiki/Saha_ionization_equation

    Let = 2.69 × 10 25 m −3, which is the Loschmidt constant, or particle density of Earth's atmosphere at standard pressure and temperature. At T {\displaystyle T} = 300 K , the ionization is essentially none: x {\displaystyle x} = 5 × 10 −115 and there would almost certainly be no ionized atoms in the volume of Earth's atmosphere.

  4. Thermosphere - Wikipedia

    en.wikipedia.org/wiki/Thermosphere

    The density of the Earth's atmosphere decreases nearly exponentially with altitude. The total mass of the atmosphere is M = ρ A H ≃ 1 kg/cm 2 within a column of one square centimeter above the ground (with ρ A = 1.29 kg/m 3 the atmospheric density on the ground at z = 0 m altitude, and H ≃ 8 km the average atmospheric scale height ).

  5. Negative temperature - Wikipedia

    en.wikipedia.org/wiki/Negative_temperature

    The two-dimensional systems of vortices confined to a finite area can form thermal equilibrium states at negative temperature, [18] [19] and indeed negative temperature states were first predicted by Onsager in his analysis of classical point vortices. [20]

  6. Total electron content - Wikipedia

    en.wikipedia.org/wiki/Total_electron_content

    TEC plot for the continental USA, made on 2013-11-24. Total electron content (TEC) is an important descriptive quantity for the ionosphere of the Earth. TEC is the total number of electrons integrated between two points, along a tube of one meter squared cross section, i.e., the electron columnar number density.

  7. Charge carrier density - Wikipedia

    en.wikipedia.org/wiki/Charge_carrier_density

    Charge carrier density, also known as carrier concentration, denotes the number of charge carriers per volume. In SI units, it is measured in m −3. As with any density, in principle it can depend on position. However, usually carrier concentration is given as a single number, and represents the average carrier density over the whole material.

  8. Electron - Wikipedia

    en.wikipedia.org/wiki/Electron

    The electron (e −, or β − in nuclear reactions) is a subatomic particle with a negative one elementary electric charge. [13] Electrons belong to the first generation of the lepton particle family, [14] and are generally thought to be elementary particles because they have no known components or substructure. [1]

  9. Fermi energy - Wikipedia

    en.wikipedia.org/wiki/Fermi_energy

    Under the free electron model, the electrons in a metal can be considered to form a Fermi gas.The number density / of conduction electrons in metals ranges between approximately 10 28 and 10 29 electrons/m 3, which is also the typical density of atoms in ordinary solid matter.