What is the definition of Unit Optical Depth?

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SUMMARY

Unit Optical Depth is defined as the measure of opacity in a medium, quantified by the equation χ = nσ, where χ represents opacity, n is the number density of absorbers, and σ is the cross section. The optical depth τ is calculated as τ = ∫(z1 to z2) χ dz, indicating the total number of photon mean-free paths between two points along a ray. This concept is crucial for understanding light propagation through various media, particularly in astrophysics and atmospheric sciences. The discussion highlights the confusion surrounding the calculation of Unit Optical Depth at a specific wavelength, emphasizing the need for clarity on the parameters involved.

PREREQUISITES
  • Understanding of optical depth and its significance in physics
  • Familiarity with the concepts of photon mean-free paths
  • Knowledge of cross-sectional area in scattering processes
  • Basic calculus for integrating optical depth equations
NEXT STEPS
  • Research the implications of optical depth in astrophysical contexts
  • Learn about the role of wavelength in determining optical properties
  • Explore the calculation of optical depth in various media
  • Study the application of the Beer-Lambert Law in light absorption
USEFUL FOR

Astronomers, physicists, and students studying light propagation in different media will benefit from this discussion, particularly those interested in the quantitative analysis of optical depth in astrophysical phenomena.

AlphaCrucis
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Homework Statement
I'm trying to calculate how far away from some object is Unit Optical Depth at some given wavelength; but i'm confused as to what exactly Unit Optical Depth is? What am i Calculating
Relevant Equations
Below
\begin{equation}
\chi = n \sigma
\end{equation}
Where Chi is the Opacity, n is the number density of absorbers (constant), and $\sigma$ is the cross section(given).

We define the optical depth is just the number of photon mean-free paths in a given physical step, i.e. if we consider a physical step:
\begin{equation}
\Delta \tau = \chi \Delta z
\end{equation}

Therefore, in traveling from location z1 to z2 along a straight-line ray, the total optical depth is
\begin{equation}
\tau = \int_{z_1}^{z_2} \chi \,dz
\end{equation}I'm trying to calculate how far away from some object is Unit Optical Depth at some given wavelength; but I'm confused as to what exactly Unit Optical Depth is? What am i calculating? I am given n and the wavelength along with the cross section
 
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