<p>Aerosol physics is actually an old topic - yet still a very vibrant one.</p>
<p>One main factor on the extinction (which sums up scattering and absorption) other than the distance (which is about constant when looking at a a particular zenith distance) is the wavelength <span class="math-container">$\lambda$</span> you look at compared to the typical aerosol particle radius <span class="math-container">$r$</span> as its ratio affects the scattering regime we look at (<span class="math-container">$\lambda \gg r, \lambda \approx r, \lambda \ll r$</span>). There's multiple papers on the aerosol influence on observations, like <a href="https://arxiv.org/pdf/0708.1364.pdf" rel="nofollow noreferrer">this (Stubbs et al) for PanSTARRS</a> or <a href="https://arxiv.org/pdf/1011.6156.pdf" rel="nofollow noreferrer">Patat et al (2018) on extinction over Paranal</a> which also looks at the temporal variability.</p>
<p>Looking at the typical aerosol concentrations (e.g. <a href="https://www.dwd.de/EN/research/observing_atmosphere/composition_atmosphere/aerosol/cont_nav/particle_size_distribution_node.html" rel="nofollow noreferrer">here by DWD</a>), it seems that the smaller particles are more abundant. Thus we are in the Rayleigh or Mie scattering regimes where the extinction is due to scattering and does not depend much on the actual particle properties other than their size. The actual absorption only becomes important for the larger particles which are the least abundant.</p>
<p>All in all this might only be half an answer, but too long for a comment and maybe gives you leads to follow-up on. If you get a hand on <a href="https://www.amazon.de/-/en/Sheldon-K-Friedlander/dp/0195129997" rel="nofollow noreferrer">Friedlander's &quot;smoke, dust and haze&quot;</a>, it might be a good read, too (especially chapters 5 and 13).</p>

CC BY-SA 4.0
2021-02-12T10:46:19.657Z
Thanks for the helpful hints and links.  In my understanding, particulates (and in particular soot or BC) are not necessarily an aersol, i.e. a mixture of liquid and solid particles, but will surely have similar (Scattering) effects. I vividly remember a related discussion in 2010 on in how far [Eyjafjallajökull's Volcanic ash](https://en.wikipedia.org/wiki/2010_eruptions_of_Eyjafjallaj%C3%B6kull) behaved.
B--rian
CC BY-SA 4.0
2021-02-12T10:56:33.577Z
Uh, the definition of aerosol is "solid or liquid particles suspended in a gas" (and where we have considerable effects which make its lifetime in the atmosphere differ greatly from the vacuum free-fall time; thus a fist-size rock falling from the sky is no aerosol, of course). However yes, soot and BC in the atmosphere are (an important) part of the atmosphere's aerosol content, especially in the near-surface region.
planetmaker
CC BY-SA 4.0
2021-02-12T11:04:42.080Z
Yeah, I just found out that your (more general) definition of aersol is the wider used one. Interestingly, some organizations distinguish between wet and dry particulates - I got carried aways with that definition.
B--rian
CC BY-SA 4.0
2021-02-12T10:39:25.607Z
2021-02-12T10:40:39.820Z
2021-02-12T10:40:39.820Z
planetmaker
<p>I am looking for a (mathematical) relationship - either empirical or theoretical - which quantifies <strong>how the visibility of celestrial objects decreases with increasing amount of <a href="https://en.wikipedia.org/wiki/Particulates" rel="nofollow noreferrer">particulates</a> in the air</strong>. I would be already happy if somebody knows such a relationship for the atmospheric light attenuation effects of <a href="https://en.wikipedia.org/wiki/Black_carbon" rel="nofollow noreferrer">black carbon</a> or soot. Those two are actually not the same as <a href="https://de.wikipedia.org/wiki/Alfred_Wiedensohler" rel="nofollow noreferrer">Alfred Wiedensohler</a> from the <a href="https://www.tropos.de/" rel="nofollow noreferrer">Leibniz Institute for Tropospheric Research</a> points out in <a href="https://www.wmo-gaw-wcc-aerosol-physics.org/files/wiedensohler.pdf" rel="nofollow noreferrer">a presentation on the topic</a>:</p>
<blockquote>
<p>Soot is carbon particles resulting from the incomplete combustion of hydrocarbons. Soot contains <a href="https://en.wikipedia.org/wiki/Polycyclic_aromatic_hydrocarbon" rel="nofollow noreferrer">polycyclic aromatic hydrocarbons</a> (PAHs) and <a href="https://en.wikipedia.org/wiki/Toxic_heavy_metal" rel="nofollow noreferrer">heavy metals</a>. Black carbon (BC) itself is neither a toxic nor a carcinogen.</p>
</blockquote>
<p>What I expect (but I am happy to be proven wrong) is that I am actually after the three constants in the following expression:</p>
<p><span class="math-container">$$ f_{\rm attenuation}(d) =  \frac{1}{k_c + k_l \cdot d + k_q \cdot d^2}$$</span></p>
<p>In this formula, <span class="math-container">$d$</span> is the distance between the light source and the observers, so in our case it would be the height of Earth's atmosphere (if we assume homogenous distribution of soot/ BC over the air column).
<span class="math-container">$k_c$</span> is called the <em>constant attenuation factor</em>, <span class="math-container">$k_l$</span> is the <em>linear attenuation factor</em>, and <span class="math-container">$k_q$</span> stands for <em>quadratic attenuation factor</em>.</p>
<p>Such an expression would already be very helpful, but if there is science on the overall effect of particulates, that would be much cooler. I am dreaming of having a formula for visible magnitude of stars with naked eye in dependence of particulate concentration (for ideal, pitch-black nights without clouds).</p>
<h3>Background</h3>
<p>My question is inspired by <a href="https://astronomy.stackexchange.com/questions/37182/what-effect-do-aircraft-have-on-night-time-visibility">What effect do aircraft have on night-time visibility?</a> which does not have an answer yet.</p>
<p>I am aware that in the <a href="https://en.wikipedia.org/wiki/Physical_oceanography" rel="nofollow noreferrer">physical oceanography</a> and in <a href="https://en.wikipedia.org/wiki/Marine_biology" rel="nofollow noreferrer">marine biology</a>, there are extensive studies on light attenuation due to BC or other dissolved substances <em>in water</em>, and most search results are on that.</p>
<h3>References and related questions</h3>
<ul>
<li>C.Liousse, H.Cachier, S.G.Jennings: <a href="https://doi.org/10.1016/0960-1686(93)90246-U" rel="nofollow noreferrer">Optical and thermal measurements of black carbon aerosol content in different environments: Variation of the specific attenuation cross-section</a> (1993)</li>
<li>H. Horovath: <a href="https://doi.org/10.1016/0960-1686(93)90104-7" rel="nofollow noreferrer">Atmospheric light absorption — A review</a>
(1993)</li>
<li>ESA on <a href="https://www.esa.int/Applications/Observing_the_Earth/Satellites_track_unusual_Saharan_dust_plume" rel="nofollow noreferrer">Desert dust plume over the Atlantic observed by Aeolus and Sentinel-5P</a></li>
</ul>

<observational-astronomy><planetary-atmosphere><light-pollution><atmospheric-effects><modeling>
Effect of particulates on the visibility of stars?
B--rian
# Effect of particulates on the visibility of stars?

(Asked by: username_0 on 2021-02-12)

I am looking for a (mathematical) relationship - either empirical or theoretical - which quantifies **how the visibility of celestrial objects decreases with increasing amount of [particulates](https://en.wikipedia.org/wiki/Particulates) in the air**. I would be already happy if somebody knows such a relationship for the atmospheric light attenuation effects of [black carbon](https://en.wikipedia.org/wiki/Black_carbon) or soot. Those two are actually not the same as [Alfred Wiedensohler](https://de.wikipedia.org/wiki/Alfred_Wiedensohler) from the [Leibniz Institute for Tropospheric Research](https://www.tropos.de/) points out in [a presentation on the topic](https://www.wmo-gaw-wcc-aerosol-physics.org/files/wiedensohler.pdf):

> Soot is carbon particles resulting from the incomplete combustion of hydrocarbons. Soot contains [polycyclic aromatic hydrocarbons](https://en.wikipedia.org/wiki/Polycyclic_aromatic_hydrocarbon) (PAHs) and [heavy metals](https://en.wikipedia.org/wiki/Toxic_heavy_metal). Black carbon (BC) itself is neither a toxic nor a carcinogen.

What I expect (but I am happy to be proven wrong) is that I am actually after the three constants in the following expression:

$$ f\_{\rm attenuation}(d) = \frac{1}{k\_c + k\_l \cdot d + k\_q \cdot d^2}$$

In this formula, $d$ is the distance between the light source and the observers, so in our case it would be the height of Earth's atmosphere (if we assume homogenous distribution of soot/ BC over the air column).
$k\_c$ is called the *constant attenuation factor*, $k\_l$ is the *linear attenuation factor*, and $k\_q$ stands for *quadratic attenuation factor*.

Such an expression would already be very helpful, but if there is science on the overall effect of particulates, that would be much cooler. I am dreaming of having a formula for visible magnitude of stars with naked eye in dependence of particulate concentration (for ideal, pitch-black nights without clouds).

### Background

My question is inspired by [What effect do aircraft have on night-time visibility?](https://astronomy.stackexchange.com/questions/37182/what-effect-do-aircraft-have-on-night-time-visibility) which does not have an answer yet.

I am aware that in the [physical oceanography](https://en.wikipedia.org/wiki/Physical_oceanography) and in [marine biology](https://en.wikipedia.org/wiki/Marine_biology), there are extensive studies on light attenuation due to BC or other dissolved substances *in water*, and most search results are on that.

### References and related questions

* C.Liousse, H.Cachier, S.G.Jennings: [Optical and thermal measurements of black carbon aerosol content in different environments: Variation of the specific attenuation cross-section](https://doi.org/10.1016/0960-1686(93)90246-U) (1993)
* H. Horovath: [Atmospheric light absorption — A review](https://doi.org/10.1016/0960-1686(93)90104-7)
  (1993)
* ESA on [Desert dust plume over the Atlantic observed by Aeolus and Sentinel-5P](https://www.esa.int/Applications/Observing_the_Earth/Satellites_track_unusual_Saharan_dust_plume)

**Tags:** observational-astronomy, planetary-atmosphere, light-pollution, atmospheric-effects, modeling


---

## 1 answers

### Answer by username_1 on 2021-02-12. Score: 2 | Accepted answer

Aerosol physics is actually an old topic - yet still a very vibrant one.

One main factor on the extinction (which sums up scattering and absorption) other than the distance (which is about constant when looking at a a particular zenith distance) is the wavelength $\lambda$ you look at compared to the typical aerosol particle radius $r$ as its ratio affects the scattering regime we look at ($\lambda \gg r, \lambda \approx r, \lambda \ll r$). There's multiple papers on the aerosol influence on observations, like [this (Stubbs et al) for PanSTARRS](https://arxiv.org/pdf/0708.1364.pdf) or [Patat et al (2018) on extinction over Paranal](https://arxiv.org/pdf/1011.6156.pdf) which also looks at the temporal variability.

Looking at the typical aerosol concentrations (e.g. [here by DWD](https://www.dwd.de/EN/research/observing_atmosphere/composition_atmosphere/aerosol/cont_nav/particle_size_distribution_node.html)), it seems that the smaller particles are more abundant. Thus we are in the Rayleigh or Mie scattering regimes where the extinction is due to scattering and does not depend much on the actual particle properties other than their size. The actual absorption only becomes important for the larger particles which are the least abundant.

All in all this might only be half an answer, but too long for a comment and maybe gives you leads to follow-up on. If you get a hand on [Friedlander's "smoke, dust and haze"](https://www.amazon.de/-/en/Sheldon-K-Friedlander/dp/0195129997), it might be a good read, too (especially chapters 5 and 13).

> **Comments:**
> **username_0**: Thanks for the helpful hints and links.  In my understanding, particulates (and in particular soot or BC) are not necessarily an aersol, i.e. a mixture of liquid and solid particles, but will surely have similar (Scattering) effects. I vividly remember a related discussion in 2010 on in how far [Eyjafjallajökull's Volcanic ash](https://en.wikipedia.org/wiki/2010_eruptions_of_Eyjafjallaj%C3%B6kull) behaved.  
> **username_1**: Uh, the definition of aerosol is "solid or liquid particles suspended in a gas" (and where we have considerable effects which make its lifetime in the atmosphere differ greatly from the vacuum free-fall time; thus a fist-size rock falling from the sky is no aerosol, of course). However yes, soot and BC in the atmosphere are (an important) part of the atmosphere's aerosol content, especially in the near-surface region.  
> **username_0**: Yeah, I just found out that your (more general) definition of aersol is the wider used one. Interestingly, some organizations distinguish between wet and dry particulates - I got carried aways with that definition.  

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