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Langley extrapolation

Langley extrapolation is a science topic covered in the lgStudy science library. This page brings together a partial reference excerpt, illustrations, worked examples, real-world applications and a short study plan, so you can understand Langley extrapolation rather than just read about it. In short: Langley extrapolation is a method for determining the Sun's irradiance at the top of the atmosphere with ground-based instrumentation, and is often used to remove the effect of the atmosphere from measurements of, for example, aerosol optical thickness or ozone. It is based on repeated measurements with a Sun photometer operated at a given location for a cloudless morning or afternoon as the Sun moves across the sky.

Langley extrapolation — main illustration
Langley extrapolation — illustration

Key takeaways

  • Langley extrapolation belongs to science; place it in that map before memorising details.
  • Learn the definition first, then one example that makes the definition concrete.
  • Connect Langley extrapolation to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of Langley extrapolation from memory before moving on to harder problems.

Reference excerpt

Langley extrapolation is a method for determining the Sun's irradiance at the top of the atmosphere with ground-based instrumentation, and is often used to remove the effect of the atmosphere from measurements of, for example, aerosol optical thickness or ozone. It is based on repeated measurements with a Sun photometer operated at a given location for a cloudless morning or afternoon as the Sun moves across the sky. It is named for American astronomer and physicist Samuel Pierpont Langley.

Theory It is known from Beer's law that, for every instantaneous measurement, the direct-Sun irradiance I is linked to the solar extraterrestrial irradiance I0 and the atmospheric optical depth τ {\displaystyle \tau } by the following equation:

where m is a geometrical factor accounting for the slant path through the atmosphere, known as the airmass factor. For a plane-parallel atmosphere, the airmass factor is simple to determine if one knows the solar zenith angle θ: m = 1/cos(θ). As time passes, the Sun moves across the sky, and therefore θ and m vary according to known astronomical laws.

By taking the logarithm of the above equation, one obtains:

and if one assumes that the atmospheric disturbance τ {\displaystyle \tau } does not change during the observations (which last for a morning or an afternoon), the plot of ln I versus m is a straight line with a slope equal to τ {\displaystyle \tau } . Then, by linear extrapolation to m = 0, one obtains I0, i.e. the Sun's radiance that would be observed by an instrument placed above the atmosphere.

The requirement for good Langley plots is a constant atmosphere (constant τ {\displaystyle \tau } ). This requirement can be fulfilled only under particular conditions, since the atmosphere is continuously changing. Needed conditions are in particular: the absence of clouds along the optical path, and the absence of variations in the atmospheric aerosol layer. Since aerosols tend to be more concentrated at low altitude, Langley extrapolation is often performed at high mountain sites. Data from NASA Glenn Research Center indicates that the Langley plot accuracy is improved if the data is taken above the tropopause.

Solar cell calibration A Langley plot can also be used as a method to calculate the performance of solar cells outside the Earth's atmosphere. At the Glenn Research Center, the performance of solar cells is measured as a function of altitude. By extrapolation, researchers determine their performance under space conditions.

Low cost LED-based photometers Sun photometers using low cost light-emitting diode (LED) detectors in place of optical interference filters and photodiodes have a relatively wide spectral response. They might be used by a globally distributed network of students and teachers to monitor atmospheric haze and aerosols, and can be calibrated using Langley extrapolation. In 2001, David Brooks and Forrest Mims were among many to propose detailed procedures to modify the Langley plot in order to account for Rayleigh scattering, and atmospheric refraction by a spherical Earth. Di Justo and Gertz compiled a handbook for using Arduino to develop these photometers in 2012. The handbook refers to τ {\displaystyle \tau } in equations (1) and (2), as the AOT (Atmospheric Optical Thickness), and the handbook refers to I0 as the EC (extraterrestrial constant). The manual suggests that once a photometer is constructed, the user waits for a clear day with few clouds, no haze and constant humidity. After the data is fit to equation (1) to find I0, the handbook suggests a daily measurement of I. Both I0 and I are obtained from the LED current (voltage across sensing resistor) by subtracting the dark current:

where V s {\displaystyle V_{s}} is the voltage while the LED is pointing at the Sun, and V d {\displaystyle V_{d}} is the voltage while the LED is kept dark. There is a misprint in the manual regarding the calculation of τ {\displaystyle \tau } from this single data point. The correct equation is:

where I 0 {\displaystyle I_{0}} was calculated on that clear and stable day using Langley extrapolation.

References

Illustrations

Langley extrapolation: Direct solar radiation, at the various wavelengths indicated in  nanometers, as measured at Niamey Niger on 24 December 2006, with a Multi-Filter Rotating Shadowband Radiometer (MFRSR). Measurements are plotted as a function of time in UTC.
Direct solar radiation, at the various wavelengths indicated in nanometers, as measured at Niamey Niger on 24 December 2006, with a Multi-Filter Rotating Shadowband Radiometer (MFRSR). Measurements are plotted as a function of time in UTC.
Langley extrapolation: Direct solar radiation as a function of secant of solar zenith angle at Niamey, Niger. December 24, 2006. From ARM data, from an MFRSR instrument. Wavelength in units of nanometers is indicated. Log is base 10.
Direct solar radiation as a function of secant of solar zenith angle at Niamey, Niger. December 24, 2006. From ARM data, from an MFRSR instrument. Wavelength in units of nanometers is indicated. Log is base 10.
Langley extrapolation: Points are Langley extrapolation to top of atmosphere of direct solar radiation measured at Niamey, Niger 24 December 2006. Compared with Planck functions with the wavelength in micrometers.
Points are Langley extrapolation to top of atmosphere of direct solar radiation measured at Niamey, Niger 24 December 2006. Compared with Planck functions with the wavelength in micrometers.

Worked examples

Example 1 — a first encounter with Langley extrapolation

Start with the simplest possible case. Write down what Langley extrapolation claims or describes in one sentence, then invent the smallest concrete situation in which that sentence is true. In science, the smallest case is usually a single object, a single equation or a single measurement. Check that every symbol or term in your sentence has a meaning in that case.

Example 2 — changing one variable

Take the situation from Example 1 and change exactly one quantity: double it, halve it, or set it to zero. Predict what should happen to Langley extrapolation before you calculate. Comparing your prediction with the result is the fastest way to find out whether you understand the idea or only the words.

Example 3 — an exam-style question

Typical questions about Langley extrapolation ask you to (a) state it precisely, (b) apply it to given data, and (c) explain a limitation. Practise writing all three answers in under five minutes; the third part is what separates a full-mark answer from an average one.

Applications of Langley extrapolation

In research
Langley extrapolation appears in science research whenever the underlying quantities have to be modelled precisely. Papers usually cite it as a starting assumption and then explore where it breaks down.
In technology and industry
Engineering practice reuses Langley extrapolation in design rules, simulations and safety margins. Knowing the idea lets you read a specification sheet and understand why the numbers look the way they do.
In the classroom
Langley extrapolation is common in secondary-school and first-year university syllabi. It links to neighbouring topics Radiometry, so understanding it makes those chapters shorter.
In everyday life
Look for Langley extrapolation outside the textbook — in sport, cooking, traffic, electronics or the sky above you. An example you found yourself is remembered far longer than one you were given.
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How to study Langley extrapolation in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what Langley extrapolation means in your own words.
  3. Compare your version with the excerpt and mark what you missed.
  4. Work through the three examples above with pen and paper.
  5. Explain Langley extrapolation out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is Langley extrapolation in simple terms?

Langley extrapolation is a method for determining the Sun's irradiance at the top of the atmosphere with ground-based instrumentation, and is often used to remove the effect of the atmosphere from measurements of, for example, aerosol optical thickness or ozone. It is based on repeated measurements…

Why does Langley extrapolation matter?

Because it connects several science ideas at once: it gives you a definition you can apply, a quantity you can calculate, and a way to check whether a result is plausible.

How should I study Langley extrapolation?

Read the excerpt, restate it from memory, then work through the examples and applications listed on this page. The five-step study plan above takes about twenty minutes.

What does this page cover?

It gives you a compact reference excerpt plus original lgStudy explanations, examples, applications and study material on Langley extrapolation.

Tags

  • Radiometry

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