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Llewelyn Robert Owen Storey

Llewelyn Robert Owen Storey is a physics 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 Llewelyn Robert Owen Storey rather than just read about it. In short: Llewelyn Robert Owen Storey (born 5 November 1927; also known as L. R.

Llewelyn Robert Owen Storey — main illustration
Llewelyn Robert Owen Storey — illustration

Key takeaways

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

Reference excerpt

Llewelyn Robert Owen Storey (born 5 November 1927; also known as L. R. O. Storey, L. R. Owen Storey, and Owen Storey) is a British physicist and electrical engineer who has worked and lived most of his adult life in France. He is known for his research on the Earth's atmosphere, especially whistlers—very low frequency (VLF) radio waves caused by lightning strikes—and the magnetosphere. He was the first person to prove whistlers are caused by lightning strikes and to deduce the plasmasphere's existence. He was heavily involved in designing scientific instruments for FR-1, a 1965 French-American satellite, and subsequent studies and experiments using data FR-1 collected.

Early life Storey was born on 5 November 1927 in Crowborough, England, United Kingdom. He received a Bachelor of Arts degree in natural sciences in 1948 and a PhD in physics in 1953, both from the University of Cambridge. He became interested in whistlers during his time as a graduate student. In fact, Storey in his 1953 PhD dissertation was the first person to realize the propagation of VLF radio waves after lightning strikes causes whistlers. Around the same time, Storey had posited the existence of whistlers meant plasma was present in Earth's atmosphere, and that it moved radio waves in the same direction as Earth's magnetic field lines. From this he deduced but was unable to conclusively prove the existence of the plasmasphere, a region of cold plasma extending from the upper ionosphere far into the magnetosphere. After obtaining his doctorate, Storey worked in England, and then Canada and the United States, before becoming an employee of the French National Centre for Scientific Research (Centre national de la recherche scientifique; CNRS) in 1959.

Career and research

FR-1: whistlers and the plasmasphere

In 1963 Storey became scientific director of the joint French-American FR-1 satellite program. He specified the satellite's scientific instruments, working in concert with Dr. Robert W. Rochelle and Sam Stevens of NASA's Goddard Space Flight Center (GSFC). FR-1 was launched on 6 December 1965. The mission objective was to study the composition and structure of the ionosphere, plasmasphere, and magnetosphere by measuring the propagation of VLF waves and the local electron density of plasma in those atmospheric layers. For the VLF wave experiments, stations located on land in Seine-Port, France (at the Sainte-Assise transmitter), and Balboa, Panama, transmitted signals at 16.8 kHz and 24 kHz, respectively, while the satellite's magnetic and electric sensors orbiting about 750 kilometres (470 mi) away analyzed the magnetic field of the received wave. Principal researchers who studied both the VLF and electron density data collected by FR-1 included Storey, as well as the French scientists Dr. M. P. Aubry of CNET and Dr. C. Renard. Aubry published his results in 1968, while Storey published initial findings in 1967 before the mission's ultimate end. Northern Irish physicist James Sayers—an electron density expert—was also involved in the electron density experiments. Data collected by FR-1 helped prove the existence of the plasmasphere. Prior to their work on FR-1, both Aubry and Storey had studied whistlers. From earlier whistler research Storey deduced the existence of the plasmasphere but was unable to conclusively prove it. In 1963 American scientist Don Carpenter and Soviet astronomer Konstantin Gringauz—independently of each other, and the latter using data from the Luna 2 spacecraft—experimentally proved the plasmasphere and plasmapause's existence, building on Storey's thinking. Aubry and Storey's post-1965 studies of FR-1 VLF and electron density data further corroborated this: VLF waves in the ionosphere occasionally passed through a thin layer of plasma into the magnetosphere, normal to the direction of Earth's magnetic field.

Later career After his work on FR-1, Storey headed his own research group which continued studying VLF waves using data gathered the satellite. It transferred to a laboratory in Orléans from its original Paris location in the early 1970s. This group's research focused on developing methods for measuring the properties of space plasmas using dipole antennas, and wave distribution function (WDF) analysis. For the plasma measurement research Storey and his group collaborated with West German and Swedish programs during the International Magnetospheric Study of 1976 to 1979, allowing them to carry out further experiments on rockets. In 1983 Storey joined the research faculty of Stanford University's Electrical Engineering Department. From 1987 to 1989 he served as a senior visiting scientist at NASA Headquarters in Washington, D.C., and then as a WDF analysis software developer at NASA's Goddard Space Flight Center. Storey retired in 1992. In 1997 he received the IEEE Heinrich Hertz Medal for his lifelong research on whistlers.

Personal life Storey is a member of the American Geophysical Union. He and his wife live in southern France; they have three children together.

See also

French space program

References

Worked examples

Example 1 — a first encounter with Llewelyn Robert Owen Storey

Start with the simplest possible case. Write down what Llewelyn Robert Owen Storey claims or describes in one sentence, then invent the smallest concrete situation in which that sentence is true. In physics, 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 Llewelyn Robert Owen Storey 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 Llewelyn Robert Owen Storey 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 Llewelyn Robert Owen Storey

In research
Llewelyn Robert Owen Storey appears in physics 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 Llewelyn Robert Owen Storey 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
Llewelyn Robert Owen Storey is common in secondary-school and first-year university syllabi. It links to neighbouring topics 1927 births, British electrical engineers, British expatriates in Canada, so understanding it makes those chapters shorter.
In everyday life
Look for Llewelyn Robert Owen Storey 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 Llewelyn Robert Owen Storey in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what Llewelyn Robert Owen Storey 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 Llewelyn Robert Owen Storey out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is Llewelyn Robert Owen Storey in simple terms?

Llewelyn Robert Owen Storey (born 5 November 1927; also known as L. R.

Why does Llewelyn Robert Owen Storey matter?

Because it connects several physics 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 Llewelyn Robert Owen Storey?

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 Llewelyn Robert Owen Storey.

Tags

  • 1927 births
  • British electrical engineers
  • British expatriates in Canada
  • British expatriates in France
  • British expatriates in the United States
  • British physicists
  • Living people

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