The Exploration of the Earth's Magnetosphere

     Illustration by Steele Hill

An educational web site by David P. Stern and Mauricio Peredo           Version of 28 June 2000

.           Your comments and suggestions may be sent to David P. Stern at audavstern@erols.com . Unless overloaded, I will try to reply. If your question concernes any file here, please name it!
        Also look up two sister sites--From Stargazers to Starships, an educational exposition of elementary astronomy, Newtonian mechanics, solar physics and spaceflight, and The Great Magnet, the Earth, a historical introduction to the Earth' magnetism, marking the 400th anniversary of William Gilbert's book "De Magnete"

    New as of October 2000: The first sections of a Spanish translation "La Exploración de la Magnetosfera Terrestre" are now available, produced by J. Méndez of Algorta, Spain. Click here to open the Spanish home page!

    You can now copy The Exploration of the Earth's Magnetosphere and its sister sites onto your own computer. Click here

Welcome!

This is the home page of an overview of space research on the Earth's environment in space. The description is non-mathematical but quite detailed, and here is what it contains:

INTRODUCTORY AND GENERAL:

    Overview.... for those not sure how to use this site.

    Introduction (former home page).... what to expect to find here.

SUMMARY FILES     .... Capsule descriptions of the different sections:

.

TABLE OF CONTENTS .... The files themselves:

1. The Magnetosphere
      1H. History: 1600--Gilbert's Terrella.
2. Magnetic Fields
      2H. History: 1820: Oersted discovers electromagnetism.
3. The Polar Aurora
      3H. History: 1860--Loomis draws map of the aurora

4. Electrons
      4H. History: 1896--J.J.Thomson discovers the electron
5. Magnetic Field Lines
      5H. History: 1846--Faraday introduces the idea of fields.
6. Electromagnetic Waves
7. Plasma
      7a. The Fluorescent Lamp: a plasma you can use
      7H. History : 1927--Irving Langmuir has a new use for the word "plasma".
8. Positive Ions
      8H. History: 1884--Svante Arrhenius proposes a theory of "ions".
9. Trapped Radiation
      9H. History: 1896--Henri Poincare shows magnetic field lines guide ions.
10. Motion of Trapped Radiation
      10H. History: 1910--Einstein introduces "adiabatic invariants".
11. Explorers 1 and 3
12. The Radiation Belts
      12H. History: 1958--Inner radiation belt is explained.
13. Energetic Particles
14. Synchronous Orbit
15. Energy
16. The Sun
      16H. History: 1843--Heinrich Schwabe discovers the sunspot cycle.
17. The Sun's Corona
18. The Solar Wind
      18A. Drawing Interplanetary Magnetic Field Lines.
     
18H. History: 1959, 1961--First direct observations of the solar wind.
19. The Magnetopause
      19H. History: 1930--the magnetic storm theory of Chapman and Ferraro.
20. Structure of the Earth's Magnetosphere
21. Lagrangian Points
22. The Wind Spacecraft
23. The Tail of the Magnetosphere
24. Substorms
25. Electric Currents from Space
      25H. History: 1903--Birkeland observes the electric currents of the polar aurora.
26. The Polar Caps
      26H. History: 1895--Birkeland's terrella experiment.
27. Auroral Imaging
28. Auroral acceleration
29. Low Polar Orbit
30. Magnetic Storms
31. Space Weather
32. Magnetospheres other than Ours
33. Cosmic Rays
34 High Energy Particles in the Universe
35. Solar Energetic Particles

ADDITIONAL MATERIAL:

For a quick rundown of what these files cover, look up the Overview file. Or else, start wherever your interest lies!


And by the way... In May '98 Exploration of the Magnetosphere was picked as one of "Ten Cool Sites" by the Exploratorium in San Francisco. It is a site worth visiting and lists many other interesting links.
  "Exploration" was also recommended by "Web Watch" in the January 1999 issue of Physics Today (page 63).

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#1.     The Magnetosphere

The Earth is a huge magnet, and its magnetic influence extends far into space.

In our everyday environment, magnetic forces are of no importance and a sensitive instrument, the compass needle, is needed to detect them. That is because we, the materials we encounter in everyday life, even the oxygen and nitrogen which we breathe, are all electrically neutral. The atoms of oxygen, for instance, contain electrons with negative electric charges and protons which are positive, but the two charges balance each other andthe electric and magnetic forces cancel. Magnetic forces have almost no effect on neutral atoms.

However, 60 miles (100 km) or more above the surface of the Earth, the natural environment is quite different. The fringes of the atmosphere at these heights are strongly heated by the Sun's x-rays and ultra-violet light (and by other causes as well), causing negative electrons to be torn off atoms and leaving the remainder of the atoms as positively charged "ions". These electrified fragments react strongly to the magnetic forces and can be steered and trapped by them.

With a suitable input of energy, such fragments can also be accelerated to high speeds, can give rise to electic currents and emit a variety of radio-type waves.

It can be shown that such free electrons and ions will be guided by the magnetic field lines (or "lines of force") which rise from near the southern (magnetic) pole and enter the Earth again near the northern pole. Electrons and ions tend to remain attached to field lines like beads on wires, though unlike beads they also slowly migrate ("drift") to neighboring "wires."

It follows that the structure of field lines near Earth determines much of the motion and behavior of the free electrons and ions found there. Satellites observing magnetic forces in space have found (figure on right) that in most directions, those lines do not go indefinitely far but are confined inside a cavity, the magnetosphere of the Earth. The space outside it is dominated by the Sun, and by the fast "solar wind" of free ions and electrons emitted by the Sun.

Next Stop: #1H.  History

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#1H.     The Earth's Magnetosphere -- History

William Gilbert
    The north-south pointing property of the compass needle was discovered in China around the year 1000, and in 1600 William Gilbert in London showed that this could be explained if the entire Earth was a huge magnet. As a model for the magnetic Earth he used a spherical magnet, which he called "terrella", the "little Earth." He moved a small compass over the surface of the terrella and demonstrated that it always pointed towards its magnetic poles.

    In the 1830s a world-wide network of magnetic observatories was set up and it was then realized that disturbances of the compass needle, which were occasionally noticed, occured on a world wide pattern. They seemed to come from outside the Earth, and Alexander von Humboldt named them magnetic storms

.

There followed more than a century of attempts to study and understand these elusive phenomena. Only after 1958, when the first scientific spacecraft were launched and when Explorers 1 and 3 discovered the radiation belt, did scientists fully appreciate the complexity of electric and magnetic phenomena that occur in the Earth's magnetic environment.

In 1959 Thomas Gold of Cornell University proposed to name that environment "magnetosphere", and this name is still used.

Further reading:

  • look up in an encyclopaedia "magnetosphere", "Gilbert, William Gilbert", "Humboldt, Alexander von".

  • William Gilberts book "De Magnete" ("On the Magnet"), originally in Latin, is available in two English translations one of them (by Dover books) still in print. See

  • Historical details and many references can be found in "A Brief History of Magnetospheric Physics Before the Spaceflight Era" by David P. Stern, Reviews of Geophysics, 27, 103-114, 1989.

Next Stop: #2.  Magnetic Fields

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#2.      Magnetic Fields

People not familiar with magnetism often view it as a somewhat mysterious property of specially treated iron or steel.

A magnetized bar has its power concentrated at two ends, its poles; they are known as its north (N) and south (S) poles, because if the bar is hung by its middle from a string, its N end tends to point northwards and its S end southwards. The N end will repel the N end of another magnet, S will repel S, but N and S attract each other. The region where this is observed is loosely called a magnetic field; a more specific look at the concept of "field" is provided in a later section.

Either pole can also attract iron objects such as pins and paper clips. That is because under the influence of a nearby magnet, each pin or paper clip becomes itself a temporary magnet, with its poles arranged in a way appropriate to magnetic attraction.

But this property of iron is a very special type
of magnetism, almost an accident of nature!

Out in space there is no magnetic iron, yet magnetism is widespread. For instance, sunspots consist of glowing hot gas, yet they are all intensely magnetic. The Earth's own magnetic powers arise deep in its interior, and temperatures there are too high for iron magnets, which lose all their power when heated to a red glow. What goes on in those magnetized regions?

It is all related to electricity.

Matter consists of electrically charged particles: each atom consists of light, negative electrons swarming around a positive nucleus. Objects with extra electrons are negatively (-) charged, while those missing some electrons are positively (+) charged. Such charging with "static electricity" may happen (sometimes unintentionally!) when objects are brushed with cloth or fur on a dry day. Experiments in the 1700s have shown that (+) repels (+), (- ) repels (-), while (+) and (-) attract each other.

Close to 1800 it was found that when the ends of a chemical "battery" were connected by a metal wire, a steady stream of electric charges flowed in that wire and heated it. That flow became known as an electric current. In a simplified view, what happens is that electrons hop from atom to atom in the metal.

In 1821 Hans Christian Oersted in Denmark found, unexpectedly, that such an electric current caused a compass needle to move. An electric current produced a magnetic force!

Andre-Marie Ampere in France soon unraveled the meaning. The fundamental nature of magnetism was not associated with magnetic poles or iron magnets, but with electric currents. The magnetic force was basically a force between electric currents (figure below):

--Two parallel currents in the same direction attract each other.

--Two parallel currents in opposite directions repel each other.

Here is how this can lead to the notion of magnetic poles.
Bend the wires into circles with constant separation (figure below):

--Two circular currents in the same direction attract each other.

--Two circular currents in opposite directions repel each other.

Replace each circle with a coil of 10, 100 or more turns, carrying the same current (figure below): the attraction or repulsion increase by an appropriate factor. In fact, each coil acts very much like a magnet with magnetic poles at each end (an "electromagnet"). Ampere guessed that each atom of iron contained a circulating current, turning it into a small magnet, and that in an iron magnet all these atomic magnets were lined up in the same direction, allowing their magnetic forces to add up.

The magnetic property becomes even stronger if a core of iron is placed inside the coils, creating an "electromagnet"; that requires enlisting the help of iron, but is not essential. In fact, some of the world's strongest magnets contain no iron, because the added benefit of iron inside an electromagnethas a definite limit, whereas the strength of the magnetic force produced directly by an electric current is only limited by engineering considerations.

In space, on the Sun and in the Earth's core, electric currents are the only source of magnetism. We loosely refer to the region of their influence as their magnetic field, a term which will be further discussed later.


Further reading: Any high-school or college text on electricity and magnetism will give a much more detailed description of magnetic fields and their properties.

Next Stop: #2H.  History

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#2H.     Magnetic Fields -- History

Until 1820, the only magnetism known was that of iron magnets
and of "lodestones", natural magnets of iron-rich ore.

It was believed that the inside of the Earth was magnetized in the same fashion, and scientists were greatly puzzled when they found that the direction of the compass needle at any place slowly shifted, decade by decade, suggesting a slow variation of the Earth's magnetic field.

How can an iron magnet produce such changes? Edmond Halley (of comet fame) ingeniously proposed that the Earth contained a number of spherical shells, one inside the other, each magnetized differently, each slowly rotating in relation to the others.

Edmond Halley

Hans Christian Oersted

Hans Christian Oersted was a professor of science at Copenhagen University. In 1820 he arranged in his home a science demonstration to friends and students. He planned to demonstrate the heating of a wire by an electric current, and also to carry out demonstrations of magnetism, for which he provided a compass needle mounted on a wooden stand.

While performing his electric demonstration, Oersted noted to his surprise that every time the electric current was switched on, the compass needle moved. He kept quiet and finished the demonstrations, but in the months that followed worked hard trying to make sense out of the new phenomenon.

Oersted's Experiment

What Oersted saw...

But he couldn't! The needle was neither attracted to the wire nor repelled from it. Instead, it tended to stand at right angles (see drawing below). In the end he published his findings (in Latin!) without any explanation.

Andre-Marie Ampere in France felt that if a current in a wire exerted a magnetic force on a compass needle, two such wires also should interact magnetically. In a series of ingenious experiments he showed that this interaction was simple and fundamental--parallel (straight) currents attract, anti-parallel currents repel. The force between two long straight parallel currents was inversely proportional to the distance between them and proportional to the intensity of the current flowing in each.
    [Only for those pursuing the math: this is not the basic force formula. Given two short parallel currents I1 and I2, flowing in wire segements of length L1 and L1 and separated by a distance R, the basic formula gives the force between them as proportional to

    I1 I2 L1 L1/R2

    (it gets further complicated if the currents flow in directions inclined to each other by some angle). To find then the force between wires of complicated shape that carry electrical currents, all these little bitty contributions to the force must be added up. For two straight wires, the final result is as above--a force inversely proportional to R, not to R2]

There thus existed two kinds of forces associated with electricity--electric and magnetic. In 1864 James Clerk Maxwell demonstrated a subtle connection between the two types of force, unexpectedly involving the velocity of light. From this connection sprang the idea that light was an electric phenomenon, the discovery of radio waves, the theory of relativity and a great deal of present-day physics. Maxwell

      Repeat Oersted's Experiment !

You will need:
  •     A pocket compass.
  •     A one-foot (30 cm) length of fairly thick wire, insulated or bare.
  •     A 1.5 volt electric cell ("battery") of size "D" or "C". The voltage is too low to cause any risk.

    1.     Lay the compass on a table, face upwards. Wait until it points north.
    2.     Lay the middle of the wire above the compass needle, also in the north-south direction (compare to the above image "What Oersted Saw"). Bend the ends of the wire so that they are close to each other.
    3.     Grab one end of the wire in one hand and press against one end of the battery.
    4.     Grab the other end with your other hand, and press momentarily against the other terminal of the battery. The needle will swing strongly by 90 degrees.
          Quickly disconnect (it is not good for the battery to draw such a large current). The needle will swing back to the north-south direction. Note that no iron is involved in producing the magnetic effect!

    5.     Repeat with the connections of the battery reversed. Note that the needle now swings 90 degrees in the opposite direction.

    6.     Take a piece of paper 2"x4" (5x10 centimeters) and fold the longer side into pleats, about 3/8" (1 centimeter) high. Put the wire on the table, its middle in the north south direction, put the pleated paper above it so that the wire is below one of the pleats, and place the compass on top of the pleats. (Or else, use a small block of wood, with a groove cut in its bottom for the wire.)
          You can now repeat the experiment with the compass above the wire (if two people perform the experiment, they need no pleats or table--one can old the compass, the other the wire and battery). Note that the needle swings in the opposite direction than when the compass was below the wire.

Futher reading:

--look up in an encyclopaedia "Halley, Edmond", "Oersted, Hans Christian", "Ampere, Andre-Marie" and "Maxwell, James Clerk."

--"From Falling Bodies to Radio Waves" by Emilio Segre, W.H. Freeman and Co., 1984, gives a very good account of the history of electricity and magnetism (and of physics up to 1895). Segre, who won the Nobel prize in physics, wrote in a clear style with many insights and anecdotes about the discoveries which laid the foundations of physics.

--"Oersted and the Discovery of Electromagnetism" by Bern Dibner (Blaisdell Publ. Co., 1962), a slim book with details about Oersted and his time.

--"Andre-Marie Ampere" by L.Pearce Williams, Scientific American January 1989, p. 90.

--"Edmond Halley, Geophysicist" by Michael E. Evans, Physics Today, February 1988, p. 41-45.

Next Stop: #3.  The Polar Aurora

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#3.               The Polar Aurora

In Alaska, Canada, Norway, Finland or northern Russia, on a clear night,
a greenish glow is often seen in the sky, known as the "Northern Lights."

aurora from space

Click here for a full size version of this image.

    During magnetic storms, the glow may move southwards, and on occasion it can be seen in much of the US. It often appears as a glow on the horizon, like the glow preceding sunrise, and has therefore become known among scientists as "aurora borealis" ("aurora" for short), Latin for "northern dawn." A similar phenomenon is also seen in southern polar regions.

  The aurora--a woodcut by Fridtjof Nansen
    To an observer, an aurora is a fascinating spectacle, constantly moving and changing. It usually consists of many near-vertical greenish rays, forming long arcs and curtains, which stretch like ribbons across the sky, often from horizon to horizon. An example is shown on the left, a woodcut by the great polar explorer Fridtjof Nansen (1861-1930). The rays constantly fade while new ones appear, and during "magnetic substorms" (described in a later section) the arcs move rapidly and expand.

The aurora

Location

    Auroral light is produced at a height of about 100 km (60 miles) when fast electrons, arriving from space, slam into atoms and molecules of the atmosphere. The computer screen displaying these words is probably lit up in a similar way, by a beam of fast electrons accelerated electrically towards it, then steered and modulated so as to form letters and pictures.

Aurora observed by
an imaging camera
aboard DE-1

    The location of auroras on Earth is strongly controlled by the Earth's magnetism. In the 19th century it was noticed that they occur most frequently in a narrow belt, the "auroral zone", which circles the magnetic pole (see history, below). Their arcs and ribbons are approximately aligned with that zone, too. The circles drawn on the left are centered on the northern magnetic pole, and the auroral "circle of fire" is evidently lined up with them.

    The magnetic connection is also demonstrated by the fact that the rays of the aurora lie along magnetic field lines, and that the Earth's magnetic field observed beneath a bright and active aurora tends to be disturbed.


Color

The green light of the aurora has a precisely defined color in the spectrum ("narrow spectral line"). Such precise colors are usually the signatures of the atoms which emit them: for instance, street lights (depending on the metal vapor they contain) usually emit either the yellow-orange light of sodium or the bluish light of mercury.

The green light of the aurora puzzled scientists for many years, since it fit no known element. It turned out to be produced by oxygen atoms, but under conditions that in our atmosphere only exist in the very rarefied upper levels. A red aurora, occasionally seen, arises at even greater heights and is also produced by electrons hitting oxygen.

Red aurora

Observing the aurora from space

Satellites nowadays observe the aurora from above, using cameras more sensitive than the human eye. On dark parts of the polar cap they can "see" aurora at most times, forming a large "auroral oval" which extends around the magnetic pole.

Aurora viewed from the Shuttle

Further reading:

--"Majestic Lights, The Aurora in Science, History and the Arts" by Robert H. Eather, American Geophysical Union, 1980.

--"The Aurora" by Candace Savage, Sierra Club, 1995.

Next Stop: #3H.  History of Early Auroral Studies

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#3H.      The Polar Aurora -- History

The term "aurora borealis" was used in 1621 by the French scientist and philosopher Pierre Gassendi, but George Siscoe has given reasons to believe it was introduced by Galileo Galilei in 1619 (p. 51 in "Majestic Lights", cited below).

Elias Loomis of Yale University compiled, in 1860, a map marking how many times in an average year were auroras observed in various locations (click here to see his map). A more accurate map was compiled in 1881 by Hermann Fritz (1830-1883) (click here to see Fritz'es map).


Birkeland and his terrella.

It was long suspected that the aurora was caused by electrons arriving from the outside and hitting the high atmosphere.

The Norwegian physicist Kristian Birkeland (1867-1917), for instance, placed a magnetized sphere, a "terrella" representing the Earth, inside a vacuum chamber, and aimed a beam of electrons towards it. He was gratified to see that the electrons were steered by the magnetic field to the vicinity of the terrella's magnetic poles.

However, it was only in 1954 that auroral electrons were actually observed, by detectors aboard a rocket launched into the aurora by Meredith, Gottlieb and Van Allen, of Van Allen's team at the University of Iowa. Carl McIlwain, another member of that team, used a 1959 rocket experiment to identify the particles as electrons of an average energy corresponding to acceleration by 6000 volts (see high energy particles).

Nowadays scientific satellites regularly cross streams of auroral electrons and measure their properties, and aurora is also observed from the ground with video cameras and special radars.

Note on Birkeland's terrella experiment

Birkeland constructed more than one terrella experiment, including (in 1913) a much larger one in a bigger chamber, shown next to his picture on the current Norwegian 200-kroner bill. That terrella was restored in 1995 by Terje Brundtland and is now demonstrated to visitors at the Auroral Observatory in Tromsø, Norway. For an article about that restoration, see here.

Futher reading:

  • "Majestic Lights, The Aurora in Science, History and the Arts" by Robert H. Eather, American Geophysical Union, 1980.

  • Some details about Birkeland's work and further references to it can be found in "A Brief History of Magnetospheric Physics Before the Spaceflight Era" by David P. Stern, Reviews of Geophysics, 27, 103-114, 1989, included on this web site.

Next Stop: #4.  Electrons

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#3a.     Auroral Frequency Map by Elias Loomis

Below is map of the frequency with which aurora is seen in various polar regions, produced in 1860 by Elias Loomis (1811-1889), professor of natural philosophy at Yale. The central band has at least "80 auroras annually".


Elias Loomis

One might expect the center of the pattern to be at the magnetic pole, but it is not: the magnetic pole is in northern Canada, while the center of the pattern is near the northwestern end of Greenland. The reason is that the Earth's field is not exactly like that of a bar magnet, but contains additional irregularities, more complex and effective mainly near the surface, not far out in space.

Click here for a full size version (144 K) of this image.

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#3b.     Auroral Frequency Map by Hermann Fritz

Shown here is a map of the frequency with which auroras are seen, produced in 1881 by the German scientist Hermann Fritz (1830-1883). The line of greatest frequency lists 100 auroras per year, while in the center of the pattern auroras are much less frequent.

Hermann Fritz

Click here for a full size version (232 K) of this image.

If the Earth's field resembled that of a simple bar magnet ("dipole"), its magnetic pole would be near the northwestern tip of Greenland, in the middle of the pattern. However, the field contains additional complex parts, whose effect does not extend as far into space, and these shift the pole actually observed on the ground to northern Canada, to the location shown on the map.

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#3c.     The Terrella


Gilbert's terrella

"Terrella" is Latin for "little Earth," the name given by William Gilbert to a magnetized sphere with which he demonstrated to Queen Elizabeth I his theory of the Earth's magnetism. By moving a small compass around the terrella and showing that it always pointed north-south, Gilbert argued that the same thing, on a vastly larger scale, was happening on Earth, and was the only reason why a compass pointed north-south.

Later scientists such as Birkeland used the name "terrella" for magnetized spheres used inside vacuum chambers, together with electron beams, to study the motion of fast charged particles near the Earth. A sophisticated terrella experiment in a vacuum chamber is currently operated by Dr. Hafez u-Rahman at the University of California at Riverside.

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#4.               Electrons

Matter consists of atoms, and atoms consist of electrically charged components--lightweight negative electrons, and positive nuclei.

How do we know?

One clue comes from the "Edison effect," discovered by Thomas Alva Edison. Imagine a glass bulb from which air has been pumped, until hardly any of it remains. In one end we embed a metal coil of wire (like that of a flashlight bulb) in the other a metal plate, as drawn. Connect now a battery between the coil and the plate, so that the former is negative and the latter is positive.

No current will flow in this circuit: some atoms or molecules may be left inside the bulb, but they are electrically neutral, and can carry no electric current. Air is an excellent insulator: electric companies can string power lines in the open air and never have to worry about currents dribbling out on their way from the power station to consumers.

Now connect a second battery to the end of the coil, so that a current flows through the coil and heats it up. As the wire begins to glow, a current begins to flow, because now negatively charged particles are emitted from the hot wire, are attracted to the positive charge on the plate and by doing so, complete the electrical circuit.

Suppose the connections of the first battery are reversed, so that now the coil is positive and the plate is negative. Then no current flows, showing that the hot wire releases only negative particles, not positive ones. These particles were named electrons

In laboratory experiments these particles were directed by electrically charged structures (similar to the "electron guns" inside TV picture tubes) to form beams. Those beams were then bent by magnets and by electrified plates, and their behavior was studied. From such experiments and others the mass of the emitted particles, which became known as "electrons", could be determined. It turned out that they were rather lightweight. The simplest atom, that of hydrogen, contains a central positive particle, a proton, and a single electron, and the proton is nearly 2000 times heavier.

Light, like heat, can also knock electrons out of a metal. If the heated coil in the drawing is replaced by a clean metal plate, and light shines onto it, electrons are again released, and current will flow in the circuit. The explanation of this phenomena, called the photoelectric effect, earned Albert Einstein the 1921 Nobel Prize.

The same process will charge a spacecraft orbiting in the sunlight positively, to a few volts. Sunlight knocks out electrons from the surface and a few manage to escape, leaving the spacecraft positively charged; the situation then stabilizes, because the positive charge prevents any more electrons from leaving.

Next Stop: #4H.  History of the Electron

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#4H.     History of the Electron

The experiment with a pumped-out glass bulb, in which an electric circuit is completed by electrons emitted from a hot wire, is credited to the US inventor Thomas Alva Edison (1847-1931), who patented it in 1883. The phenomenon is known as the "Edison effect" and many electronic devices use it nowadays.

Experiments with beams of negative particles were performed in Britain by Joseph John ("J.J.") Thomson, and led to his conclusion in 1897 that they consisted of lightweight particles with a negative electric charge, nowadays known as electrons. Thomson was awarded the 1906 Nobel Prize.

The word "elektron" in Greek means amber, the yellow fossilized resin of evergreen trees, a "natural plastic material" already known to the ancient Greeks. It was known that when amber was rubbed with dry cloth--producing what now one would call static electricity--it could attract light objects, such as bits of paper.

J.J. Thomson
William Gilbert, a physician who lived in London at the time of Queen Elizabeth I and Shakespeare, studied magnetic phenomena and demonstrated that the Earth itself was a huge magnet, by means of his "terrella" experiment. But he also studied the attraction produced when materials such as amber were rubbed, and named it the "electric" attraction. From that came the word "electricity" and all others derived from it.

During the 1800s it became evident that electric charge had a natural unit, which could not be subdivided any further, and in 1891 Johnstone Stoney proposed to name it "electron." When J.J. Thomson discovered the light particle which carried that charge, the name "electron" was applied to it. The many applications of electrons moving in a near-vacuum or inside semiconductors were later dubbed "electronics."

Further reading:

  • To mark the 100th anniversary of the discovery of the electron, the Center for History of Physics of the American Institute of Physics has created on the world wide web a suitable exhibit: http://www.aip.org/history/electron.

  • Sir George Thomson, J. J. Thomson's son, was a renowned physicist in his own right and won the Nobel prize in 1937. On the 70th anniversary of the discovery of the electron he wrote about that discovery and about later developments where electrons were discovered to act sometimes like waves: "The Septuagenarian Electron", Physics Today, May 1967, 55-61

  • The story of J. J. Thomson is also briefly given in the first chapter of "From X-Rays to Quarks" by Emilio Segre (W.H. Freeman and Co., 1980). Segre was a physicist who won the 1959 Nobel Prize and his concise history of modern physics is filled with insights and stories, some of them drawn from his own experience.

Next Stop: #5.  Magnetic Field Lines

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#5.               Magnetic Field Lines

When researchers map the three-dimensional flow of a river around a bridge pier, or of wind around the wing of an airplane (picture below), they use streamlines, lines that trace the flow of particles of water or air.

Magnetic field lines similarly describe the structure of magnetic fields in three dimensions.They are defined as follows. If at any point on such a line we place an ideal compass needle, free to turn in any direction (unlike the usual compass needle, which stays horizontal--such needles exist, see bottom of page) then the needle will always point along the field line (drawing below).

Field lines converge where the magnetic force is strong, and spread out where it is weak. For instance, in a compact bar magnet or "dipole," field lines spread out from one pole and converge towards the other, and of course, the magnetic force is strongest near the poles where they come together. The behavior of field lines in the Earth's magnetic field is very similar.

Field lines were introduced by Michael Faraday (see history), who named them "lines of force." For many years they were viewed as merely a way to visualize magnetic fields, and electrical engineers usually preferred other ways, mathematically more convenient. Not so in space, however, where magnetic field lines are fundamental to the way free electrons and ions move. These electrically charged particles tend to become attached to the field lines on which they reside, spiralling around them while sliding along them, like beads on a wire (drawing below).

Because of this attachment, the behavior of electrified gas ("plasma") in space, a gas of free ions and electrons, is dictated by the structure of field lines: electric currents, for instance, find it easiest to flow along such lines. Indeed, the role of field lines in a plasma resembles that of grain in wood: just as the grain is the "easy" direction along which wood splits most readily, so the direction of field lines is the one along which particles, electric currents, heat and certain types of waves prefer to flow.

Exploring further

A small bar magnet, on gimbals that allow it to point in any direction in space, can be procured from its manufacturer, Cochranes of Oxford, Ltd., Leafield, Oxford OX8 5NT, England. Two types are available, Mark 1 with jewelled bearings for $36.60, Mark 2 with simple bearings for $12.65. For details see their web site:
    http://www.cochranes.co.uk/BNRVP30/edu5.htm

Next Stop: #5H.  Field Lines--History

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#5H.     Magnetic Field Lines -- History

Michael Faraday
Magnetic field lines were introduced by Michael Faraday (1791-1867) who named them "lines of force." Faraday was one of the great discoverers in electricity and magnetism, responsible for the principles by which electric generators and transformers work, as well as for the foundations of electrochemistry.

The son of a blacksmith, Faraday was apprenticed to a bookbinder and often read books brought in for rebinding. Luckily for science, one of those was the volume of the Encyclopaedia Britannica with the article about "electricity." His interest drove him to popular lectures given by Humphrey Davy, Britain's leading chemist ("he lived in the odium/of having discovered sodium"), and when Davy needed an assistant, Faraday landed the job on the strength of notes he had kept of Davy's lectures. There followed a lifelong career in physics and chemistry, with many notable achievements.

Maxwell
    Most scientists nowadays view field lines as intangible abstractions, useful only for describing magnetic fields. Faraday, however, felt that they represented more, that space containing magnetic "lines of force" was no longer empty but acquired certain physical properties. Faraday's younger colleague James Clerk Maxwell, a mathematical physicist of enormous creative insight, fleshed out these ideas in rigorous mathematical terms, and "Maxwell's equations" are now the cornerstone of electromagnetic theory.

Following Maxwell, we nowadays call a space modified by the presence of magnetic field lines a "magnetic field": if a bar magnet is placed there, it will experience magnetic forces, but the field exists even when no magnet is present. Similarly, an "electric field" is the space in which electric forces may be sensed--for instance between metal objects charged (+) and (-) by a battery, as in the drawing accompanying the discussion of the electron.

Maxwell also showed (perhaps his greatest achievement) that an "electromagnetic wave" was possible, a rapid interplay of electric and magnetic fields spreading with the velocity of light. Maxwell correctly guessed that light was in fact such a wave, that it was basically an electromagnetic phenomenon, and with this his equations paved the way to a much deeper understanding of optics, the science of light.

Maxwell's younger colleague, the German Heinrich Hertz, calculated in 1886 that waves of this type would be broadcast by a rapidly alternating current in a short antenna. He then obtained such a current from an electric spark (which does produce a fast back-and-forth oscillation of electric charge) and demonstrated his "Hertzian waves" experimentally. His work was continued by scientists all over the world--e.g. by the Russian Alexander Stepanovich Popov who around 1895 detected radio waves from lightning (a natural spark!), and by the Italian Gugliemo Marconi who, at about the same time, developed the first commercial radio applications.

The waves that carry radio and television, microwaves, infra-red, visible light, ultra-violet, x-rays and gamma rays are all variations of the same basic process envisioned by Maxwell, namely, they all belong to the family of electromagnetic waves.

It may seem strange that empty space can be modified by electric and magnetic influences, as the field concept proposes. Yet it allows one to understand light and radio waves, and also to retain the conservation of energy. When a transmitter on a spacecraft broadcasts a radio signal, most of that signal spreads out into space and never reaches Earth. Is its energy lost? No, it now resides in an ever-spreading electromagnetic field, associated with the radio wave.

Next Stop: #6.  Electromagnetic Waves

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#6.     Electromagnetic Waves

Perhaps the greatest theoretical achievement of physics in the 19th century was the discovery of electromagnetic waves. The first hint was an unexpected connection between electric phenomena and the velocity of light.

Electric forces in nature come in two kinds. First, there is the electric attraction or repulsion between (+) and (-) electric charges. It is possible to use this to define a unit of electric charge, as the charge which repels a similar charge at a distance of, say, 1 meter, with a force of unit strength (actual formulas make this precise).

But second, there is also the attraction and repulsion between parallel electric currents. One could then define the unit of current, as the current which, when flowing in a straight wire, attracts a similar current in a parallel wire 1 meter away with a force of unit strength, for every meter of the wires' length.

But electric current and charge are related! We could have just as well based the unit of current on the unit of charge--say, as the current in which one unit of charge passes each second through any cross section of the wire. This second definition turns out to be quite different, and if meters and seconds are used in all definitions, the ratio of the two units of current turns out to be the speed of light, 300,000,000 meters per second.

In Faraday's time the speed of light was known, although not as accurately as it is today. It was first derived around 1676 by Ole (Olaus) Roemer, a Danish astronomer working in Paris. Roemer tried to predict eclipses of Jupiter's moon Io (mentioned later here in an altogether different connection) and he found a difference between actual and predicted eclipse times, which grew and then decreased again as the Earth circled the Sun. He correctly guessed the reason, namely, as the Earth moved in its orbit, its distance to Jupiter also went up and down, and light needed extra time to cover the extra distance.

But what was the meaning of the link between electricity and light?

Remember the idea of Faraday which evolved into the "magnetic field" concept--that space in which magnetic forces may be observed is somehow changed? Faraday also showed that a magnetic field which varied in time--like the one produced by an alternating current (AC)--could drive electric currents, if (say) copper wires were placed in it in the appropriate way. That was "magnetic induction," the phenomenon on which electric transformers are based.

So, magnetic fields could produce electric currents, and we already know that electric currents produce magnetic fields. Would it perhaps be possible for space to support a wave motion alternating between the two? Sort of:

magnetic field ---> electric current ---> magnetic field ---> electric current ---> ...

There was one stumbling block. Such a wave could not exist in empty space, because empty space contained no copper wires and could not carry the currents needed to complete the above cycle. A brilliant young Scotsman, James Clerk Maxwell, solved the riddle in 1861 by proposing that the equations of electricity needed one more term, representing an electric current which could travel through empty space, but only for very fast oscillations.

With that term added (the "displacement current"), the equations of electricity and magnetism allowed a wave to exist, propagating at the speed of light. The drawing below illustrates such a wave--green is the magnetic part, blue the electric part--the term Maxwell added. The wave is drawn propagating just along one line. Actually it fills space, but it would be hard to draw that.

 Electromagnetic Wave (see text above)

Maxwell proposed that it indeed was light. There had been earlier hints--as noted above, the velocity of light had appeared unexpectedly in the equations of electricity and magnetism--and further studies confirmed it. For instance, if a beam of light hits the side of a glass prism, only part of it enters--another part gets reflected. Maxwell's theory correctly predicted properties of the reflected beam.

Then Heinrich Hertz in Germany showed that an electric current bouncing back and forth in a wire (nowadays it would be called an "antenna") could be the source of such waves. (The current also produces a magnetic field in accordance with Ampere's law, but that field decreases rapidly with distance.) Electric sparks create such back-and-forth currents when they jump across a gap--hence the crackling caused by lightning on AM radio--and Hertz in 1886 used such sparks to send a radio signal across his lab. Later the Italian Marconi, with more sensitive detectors, extended the range of radio reception, and in 1903 detected signals from Europe as far as Cape Cod, Massachussets.

It was presumed that light from the hot wire of a lightbulb was emitted because the heat caused electrons to bounce back and forth rapidly, turning each into a tiny antenna. When physicists tried to follow that idea, however, they found that the familiar laws of nature had to be modified on the scale of atomic sizes. That was how quantum theory originated.

Gradually other electromagnetic waves were found The wave nature of light causes different colors to be reflected differently by a surface ruled in fine parallel scratches--which is why a compact laser disk (for music or computer use) shimmers in all colors of the rainbow. The orderly rows of atoms in a crystal also form parallel lines but spaced much more closely, and they turned out to have the same effect on X-rays, showing that X-rays, like light, also were electromagnetic waves, but of a much shorter wavelength. Later it was found that beams of electrons in a magnetic field, inside a vacuum tube, could become unstable and emit waves longer than light: the magnetron tube where this occured was a top-secret radar device in World War II, and it later made the microwave oven possible.

Electromagnetic waves led to radio and television, and to a huge electronic industry. But they are also generated in space--by unstable electron beams in the magnetosphere, as well as at the Sun and in the far-away universe, telling us about energetic particles in distant space, or else teasing us with unresolved mysteries. You can find more about this in the section on high energy particles.

Next Stop: #7.  Plasma


Authors and Curators:
  • David P. Stern - NASA/GSFC Code 695 (u5dps@lepvax.gsfc.nasa.gov)
  • Mauricio Peredo - Raytheon STX Corporation (peredo@istp1.gsfc.nasa.gov)

This joined-up file created June 9, 2001