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    • https://phys.libretexts.org/Bookshelves/Astronomy__Cosmology/Stellar_Atmospheres_(Tatum)/05%3A_Absorption_Scattering_Extinction_and_the_Equation_of_Transfer/5.02%3A_Absorption
      At a level in the atmosphere higher by a distance dx, the specific intensity has dropped, as a result of absorption, to I+dI. (Here dI, by the convention of differential calculus, means ...At a level in the atmosphere higher by a distance dx, the specific intensity has dropped, as a result of absorption, to I+dI. (Here dI, by the convention of differential calculus, means the increase in I, and it is in this case negative. The quantity dx, which is positive, is the decrease in I.) The linear absorption coefficient α is defined such that the fractional decrease in the specific intensity over a distance dx is given by

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