SED deviation from Black Body - real objects

In summary, estimating SED deviations from Planck's law can be done with a modest set of input parameters, but the accuracy will depend on the complexity of the material and the accuracy of the data used. In some cases, brute observation may be necessary for more accurate results.
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Nereid
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You heat an ideal material (solid, liquid, gas) and it emits electromagnetic radiation, with a spectral energy distribution (SED) following that of a "black body", per Planck.

You heat a homogeneous real material (a lump of iron, a body of water, some hydrogen; things like dust with a wide range of sizes suspended in a gas of mixed composition have their own complications) and the SED deviates from Planck.

To what extent can these deviations be estimated, from a modest set of input parameters (derivable 'from first principles'?)? How broad is the range of applicability of these estimates (e.g. SED BB deviations to the 10%/1%/ppm level? state of matter? composition? temperature?)? I'm assuming thermodynamic equilibrium, etc. In what circumstances is it necessary to resort to 'brute observation' (measure the SED), as a priori estimation is known to be 'wrong' (or, more likely, able to reliably estimate only wide ranges)?

And what happens when you have a plasma?
 
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Is there a simple set of parameters that can be used to estimate the SED in this case?

The answer to your question depends on the complexity of the material, its composition, and the temperature. Generally speaking, if the material is homogeneous and its composition is known, then it is possible to estimate the SED deviations from Planck's law to a certain degree. This estimation can be done using theoretical models or numerical simulations. The accuracy of the estimation will depend on how well the material properties (such as absorption coefficients, emission coefficients, etc.) are known.

If the material is composed of multiple components with varying temperatures, it is more difficult to accurately estimate the SED deviations. In this case, it may be necessary to rely on brute observation to obtain accurate SED data.

When dealing with plasmas, the SED can be estimated by taking into account the various components of the plasma (electrons, ions, atoms, molecules, etc.). The SED can also be estimated using numerical simulations, which take into account the interactions between the particles in the plasma. However, the accuracy of these estimates can vary depending on the accuracy of the data used to build the models.
 
  • #3


The deviations in the SED from a black body can be estimated to a certain extent using input parameters such as temperature, state of matter, composition, and size distribution. These parameters can be derived from first principles, such as thermodynamic equations and material properties. However, the accuracy of these estimates may vary depending on the complexity of the material and the precision of the input parameters.

The range of applicability of these estimates also depends on the level of deviation being considered. At a larger scale, such as the 10% or 1% level, these estimates may be more reliable and applicable to a wider range of materials. However, at smaller scales, such as the ppm level, the deviations may be more difficult to estimate accurately and may only be applicable to a limited range of materials.

In certain circumstances, it may be necessary to rely on "brute observation" to measure the SED of a real material, particularly when the deviations from a black body are expected to be significant. This could be due to the complexity of the material or the limitations of the input parameters used in the estimation.

When dealing with a plasma, the deviations from a black body can be even more significant. This is because plasmas are highly ionized and have a wide range of energy levels, resulting in a complex SED that cannot be accurately estimated using simple input parameters. In these cases, brute observation is often necessary to determine the SED of the plasma.

Overall, the estimation of SED deviations from a black body is a complex task that requires a thorough understanding of the material and its properties. While some estimates can be derived from first principles, the accuracy and applicability of these estimates may vary depending on the specific circumstances. In cases where accuracy is critical, brute observation may be the most reliable method for determining the SED of a real material.
 

1. What is the SED deviation from Black Body?

The SED (Spectral Energy Distribution) deviation from Black Body refers to the difference between the actual spectral energy distribution of an object and the theoretical black body curve. It is a measure of how well a real object emits and absorbs radiation compared to a perfect black body.

2. Why do real objects deviate from black body behavior?

Real objects deviate from black body behavior due to several factors such as the composition, temperature, and physical properties of the object. For example, the presence of different materials, such as dust or gas, can affect the emission and absorption of radiation, causing a deviation from the black body curve.

3. How is SED deviation from Black Body measured and calculated?

SED deviation from Black Body is measured by comparing the actual spectral energy distribution of an object with the theoretical black body curve. It can be calculated by using specialized instruments, such as spectrometers, to measure the emission and absorption of radiation at different wavelengths and then comparing it to the expected curve for a black body at the same temperature.

4. What are the implications of SED deviation from Black Body?

The SED deviation from Black Body can provide valuable information about the physical properties and composition of an object. It can also help us understand the mechanisms behind the emission and absorption of radiation in different materials and environments. Additionally, studying the SED deviation from Black Body can aid in the development of more accurate models and theories for various astrophysical phenomena.

5. How does the SED deviation from Black Body affect our understanding of the universe?

The SED deviation from Black Body is an essential aspect of astrophysics and plays a crucial role in our understanding of the universe. By studying the deviations in the spectral energy distribution of different objects, we can gain insights into the processes that shape our universe, such as the formation and evolution of stars, galaxies, and other cosmic structures. It also allows us to make more accurate measurements and predictions about the behavior of the universe as a whole.

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