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New machines for fusion research | Thomas Klinger | TEDxBrussels

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    What is behind me
    is the powerhouse of the Universe.
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    It is just a conventional star.
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    It is our Sun.
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    And this power station
    has been running for billions of years,
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    reliably delivering energy to us
    and to the rest of the Universe
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    just by light emission.
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    So, that's a very nice thing,
    and it obviously runs,
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    and the mechanism
    through which it runs is fusion,
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    and I'm going to explain to you
    something about that.
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    But I will also ask the question:
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    can we bring this mechanism
    on Earth directly?
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    And the answer is no, by no means.
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    The Sun is too big, the Sun is too hot,
    the Sun is too dense,
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    everything speaks against that;
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    but... and the story about the but:
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    we have to build machines,
    clever machines;
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    we, humans have to build machines
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    in order to mimic this process,
    in order to bring it on Earth.
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    So, for that, we have to understand
    a few little things of physics.
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    Don't be afraid.
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    You have to carefully distinguish
    between fission and fusion.
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    Fission is splitting heavy nuclei;
    fusion is fusing light nuclei.
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    And they both belong to the same process:
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    it's a conversion of mass into energy,
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    and that's Einstein's
    famous formula E=mc²,
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    and that's the common mechanism.
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    And this energy is released just by speed,
    by kinetic energy, by heat in other words.
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    So it generates heat.
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    And that's what we would like
    to make use of.
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    And for that, we have to use a trick.
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    Instead of using conventional hydrogen,
    we use versions of hydrogen.
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    And these two so-called isotopes
    are called deuterium and tritium.
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    Deuterium is just heavy hydrogen,
    tritium is super heavy hydrogen.
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    They both are actually hydrogen isotopes,
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    they behave like hydrogen,
    just the mass is different.
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    And you can much more easily fuse them
    than conventional hydrogen,
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    than the hydrogen we know
    from the everyday world.
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    And when we fuse them, they collide,
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    and in the collision, they generate
    a helium nucleus, an alpha particle,
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    and a neutron, and lots of energy.
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    And that's the process we would like
    to make use of; we, fusion scientists.
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    And in order to get a feeling
    what is this fuel about:
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    fusing one gram of deuterium-tritium
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    releases the same energy
    as burning 10 million grams of coal.
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    And so, that's a fantastic fuel.
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    And so, you can say: is it available
    on Earth, or is it just a dream?
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    And the answer is yes,
    it is basically available.
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    So, deuterium is found just in seawater,
    in a low concentration,
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    but we do not need much.
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    Tritium is available on Earth
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    by making use of a mechanism
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    that generates tritium from lithium.
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    And so, if you now
    put everything together,
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    you can say that a half-filled
    bath tub of water and an accumulator -
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    here, there's a lithium-ion
    accumulator in this mobile phone -
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    would release enough energy
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    to supply an average European
    for 25 years with electric energy.
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    That's of course, a big, big promise.
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    How to make it happen?
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    And this big promise has driven
    mankind for 50 years already
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    to explore how it can work.
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    And this diagram here shows
    the early days of fusion research.
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    It's from the 1950s,
    so that's from Los Alamos [Lab]
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    and they built a device, a machine.
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    And there is this ring in the background -
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    at the center of the photo,
    there's a ring with a purple glow -
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    and this ring, together with
    what's surrounded by
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    was called the Perhapsatron -
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    and that's because the scientists
    didn't know if it would work at all.
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    It worked somehow, but not sufficiently,
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    because the very basic problem of fusion
    is fusion is very easy to do.
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    The fundamental nuclear process
    is known, and it's easy to do.
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    The exercise is to make a lot
    of fusion processes at the same time.
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    Again, so we need a lot of fusion
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    in order to generate
    substantial amounts of energy.
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    And so, it became obvious
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    that one has to work on different things
    in order to build the right machine.
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    The Perhapsatron not being
    the right machine was discarded.
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    Many, many others followed,
    other generations followed,
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    and I would like to give you
    an update on the current status.
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    So, the magnetic field is very important:
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    you have to make use of the magnetic field
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    in order to confine this super hot gas
    which we call plasma.
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    And you might have seen a plasma
    already in reality
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    if you have seen the Northern Lights
    or an Aurora Borealis.
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    That's a photo through
    the window of an airplane
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    of the Aurora Borealis
    over the Northern Pole.
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    The structure of the Aurora Borealis -
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    this stripe-like structure is given
    by the magnetic field of the Earth.
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    So this is naturally occurring.
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    And the plasma is actually the ingredient
    that's the boiling soup
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    that makes fusion happen
    so many times as it should be
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    in order to really gain energy.
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    That's in the kind of standard machine.
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    We are building a fusion science:
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    it is called tokamak -
    tokamak not tomahawk;
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    that's a big difference!
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    The tokamak consists
    of superconducting coils
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    in which a very strong current is running.
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    It is also based on a strong current
    running in the actual plasma,
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    and the plasma is ring-shaped.
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    So this purple ring there,
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    or this magenta ring shown there,
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    is the actual plasma
    that is attached to the magnetic field.
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    That's the basic principle of a tokamak,
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    and nowadays,
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    we are brave enough
    in fusion research to build big machines,
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    because they must be big in order to have
    a lot of fusion reactions.
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    The biggest tokamak in the world,
    now under construction,
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    is the tokamak ITER
    in the South of France.
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    And it's a world tokamak in a sense.
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    It's not only a big tokamak,
    the biggest tokamak in the world,
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    but it's also a world project,
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    because in the ITER project,
    half of mankind is involved:
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    China, the USA, Russia, the EU,
    India, Japan, and South Korea.
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    They're all joining forces
    in order to build
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    this really big superconducting
    tokamak in the South of France.
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    And this machine is going
    to start operating in 2025.
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    This is a big, big project.
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    There's another concept
    which is called a stellarator.
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    Stellarator means bringing
    the [power of] a star on Earth.
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    And here, in blue again,
    the magnets are shown
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    that generate a magnetic field.
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    And in yellow,
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    that's the shape of the plasma
    given by the magnetic field geometry.
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    Stellarators need optimization.
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    What does optimization mean?
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    Optimization means
    setting up a number of criteria:
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    good plasma stability,
    improved heat insulation,
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    equilibrium, confinement,
    things like that.
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    And you cast everything,
    all these requirements,
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    in a set of computer codes -
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    very massive computer codes
    with a lot of plasma theory in it -
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    and then you have to do
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    all these horribly complicated
    calculations using supercomputers.
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    And the supercomputer
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    that has calculated the Wendelstein 7-X -
    that's our stellarator -
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    was the Cray X-MP.
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    This device has more computer power
    than the Cray X-MP -
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    this goes back to the mid 80s,
    and supercomputers look different now -
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    but nevertheless,
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    the computing power was sufficient
    to determine the shape of the coils.
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    These calculations were repeated
    and confirmed many times,
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    and so we are pretty confident
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    that we have found
    the right magnetic field.
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    The Wendelstein 7-X stellarator
    consists now of the following elements:
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    the plasma - so that's
    the shape of the plasma,
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    it looks a little bit like
    a twisted tire of a bicycle -
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    the magnetic field coils,
    these calculated magnetic field coils;
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    another set of coils
    to change the magnetic field a little bit;
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    a massive steel structure
    that carries these coils -
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    each coil weighs six tonnes
    and has a diameter of three meters -
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    and of course,
    also many pipes and connectors
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    to connect the magnet system together;
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    and also an outer vessel -
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    it's a massive steel vessel
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    because the coils
    have to be operated in vacuum
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    since, for superconductivity,
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    you have to cool down the coils
    to minus 270 degrees centigrade.
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    That's then the outer shape
    of the machine.
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    It looks a little bit like a spaceship,
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    So the "Science" magazine wrote
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    it looks like
    Han Solo’s Millennium Falcon,
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    and they also wrote
    this machine was designed in hell.
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    It's all not true;
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    it's just a kind of engineering exercise,
    and that's the machine in reality.
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    And you also have
    the comparison to a person.
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    It is a complicated machine.
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    Four hundred technicians,
    engineers, and scientists
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    have worked 20 years to build the machine
    in Greifswald, Northern Germany.
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    Twenty years, one million assembly hours.
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    And the machine is running.
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    We were pushing the button,
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    and the physicists in the center
    did the job for us.
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    In the inset, you also see the plasma.
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    The plasma is glowing nicely
    bluish and reddish.
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    These are different stages
    of the plasma development.
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    The machine runs perfectly fine.
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    That's very satisfying
    after 20 years of construction,
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    and we are putting a lot of hope
    on the performance of this machine.
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    And here's the performance:
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    0.01 grams of hydrogen
    were injected into the vessel,
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    heated up with 4 million watts
    of microwave power
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    to 100 million degrees centigrade
    for the electrons
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    and 20 million degrees centigrade
    for the hydrogen.
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    That wasn't that bad
    for the first step of the machine.
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    We have to increase
    the particle density by a factor of 5,
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    which sounds easy,
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    but it needs more heating power.
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    We are currently upgrading the machine
    to increase the heating power
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    to ten million watts, to ten megawatts,
    for ten-second pulses,
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    and later on, also for longer ones.
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    I would like to conclude.
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    I would like to make
    a case here for fusion.
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    Fusion is clean;
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    it has no CO₂ emission -
    keyword 'climate change';
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    no long term waste -
    different from fission;
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    it is abundant - enough fusion fuel
    for millions of years;
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    and it's accessible to everybody -
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    so nobody owns the fusion fuel,
    which is very important, of course;
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    it's safe - there are
    no catastrophic failures possible;
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    and it's economic -
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    the machines are expensive,
    but the fuel cost is essentially zero.
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    Two key machines in the world are:
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    Wendelstein 7-X -
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    here the mission is to help create
    a hydrogen plasma for 30 minutes,
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    and this has never been done before,
    the standard is a few seconds up to now;
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    and the ITER mission
    is to create a fusion plasma
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    which generates ten times more energy
    than needed to create plasma.
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    I think that will be a major breakthrough,
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    and then, we have
    a new primary energy source,
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    and I should say
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    this is the only new primary energy source
    mankind is working on.
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    Thank you for your attention.
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    (Applause)
Title:
New machines for fusion research | Thomas Klinger | TEDxBrussels
Description:

This talk was given at a TEDx event using the TED conference format but independently organized by a local community. Learn more at http://ted.com/tedx

Plasma physicist Thomas Klinger is dealing with the fundamental principles of a future power plant, which – like the Sun – will produce energy from the fusion of light atomic nuclei. Embedded in an international endeavor, this requires the design and construction of large research facilities such as ITER and Wendelstein 7-X to develop the knowledge base for the exploitation of a new clean and abundant primary energy source.

Thomas Klinger is head of the "Stellarator Dynamics and Transport" Division and since 2005 scientific director of the project "Wendelstein 7-X" as well as member of the Directorate of IPP.

The Wendelstein 7-X (W7-X) reactor is an experimental stellarator (nuclear fusion reactor) built in Greifswald, Germany, by the Max Planck Institute of Plasma Physics (IPP).

In April 2001, he was appointed as Scientific Member of the Max-Planck Society and Director at the Max-Planck-Institute of Plasma Physics (IPP) in Greifswald.

After a research period in France he obtained his PhD in 1994 with a thesis on non-linear plasma dynamics. As a research assistant at the University of Kiel, Klinger was concerned with drift wave turbulence and nonlinear plasma structures. As visiting scientist he conducted research at the Alfvén Laboratory in Stockholm, the Centre de Physique Théorique and the Université Aix-Provence in Marseille and the Max-Planck-Institute of Plasma Physics in Garching. He obtained his habilitation in 1998 with a thesis on the control of plasma instabilities. Shortly thereafter he was appointed Professor of Experimental Physics at the Ernst-Moritz Arndt University, Greifswald, where he has headed the Institute of Physics as chair from 2000 till 2001.

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Video Language:
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Duration:
11:21
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