This discovery made ITER possible
Thursday 27 October 2022
October 2022, Press Release from the Max Planck Institute for Plasma Physics (IPP): 40 years of H-mode Forty
years ago, physicists at the Max Planck Institute for Plasma Physics
found a new plasma state that could be particularly suitable for energy
production: the H-mode. On 8 November 1982, the corresponding paper was
published, giving fusion research a worldwide boost. To this day, the
investigation of the H-mode is one of their most important fields of
work. The breakthrough came on a Thursday when – as often before –
plasmas with neutral beam heating were to be studied at high
temperatures. These plasmas were of a stubborn uniformity. "But in the
middle of the series, the important plasma parameters suddenly changed.
All the scientists in the ASDEX control room realised that something
extraordinary had happened," Prof. Dr. Friedrich Wagner recalled, who
was responsible for this area of research at ASDEX at the time. At first
on this 4 February 1982, many believed that they were dealing with
"dirty discharges" and large sawtooths, i.e. internal energy
relaxations. In fact, Prof. Wagner and his colleagues at the Max Planck
Institute for Plasma Physics (IPP) in Garching made one of the most
important discoveries in nuclear fusion research to date: they found the
H-mode. The corresponding article appeared in the journal
"Physical Review Letters" 40 years ago, on 8 November 1982. It ended a
long phase of stagnation and disappointment in the fusion community
about the usefulness of neutral beam heating. It is true that in the
1970s researchers had been able to heat plasmas to remarkable ion
temperatures of seven kiloelectronvolts, which briefly triggered a
veritable euphoria. But it soon turned out that the high plasma
temperatures were bought by a decrease in energy confinement. It was
like heating a room vigorously while simultaneously opening the windows.
This plasma behaviour posed a threat to the further development of a
fusion power plant. Many in the fusion community thought the H-mode was a measurement error. Today,
this unfavourable operating state is called L-mode (Low-Confinement
Mode). Wagner's discovery at ASDEX, the predecessor of the current
Garching experiment ASDEX Upgrade, is called High-Confinement Mode, or
H-mode for short. That this was actually a new plasma state was
initially disputed. "I went to the Varenna Summer School in Italy in
June 1982, where I presented our results publicly for the first time.
American colleagues in particular spread the word afterwards that we
were not measuring the plasma flow correctly in ASDEX," Prof. Wagner
stated, who later became director at IPP. It was only at the next
important symposium in September in Baltimore that he convinced his
colleagues after they had "grilled" him in an hour-long discussion
beforehand. A little later, they too were able to produce the new plasma
state in their facilities. "The discovery of the H-mode is what
made ITER possible in the first place," Prof. Dr. Elisabeth Wolfrum
explained, who continues research on the H-mode at IPP today. ITER, the
largest fusion device in the world, is currently being built in
Cadarache in southern France. It is designed to generate ten times more
power from fusion plasma than is supplied in heating power. The fact
that ITER is modelled on ASDEX and also ASDEX Upgrade is also due to the
H-mode. This plasma state first appeared in ASDEX because the plasma in
the donut-shaped vacuum vessel of the tokamak type was shaped for the
first time not round, but pointed. Physicists call the tip the X-point.
This is where excess energy is guided into the divertor, more or less
the ash box of a fusion reactor. Today, this design is standard in all
fusion facilities that use magnetic fields to confine the plasma. The H-mode leads to the formation of an insulating layer at the plasma edge Shortly
after the discovery of the H-mode, it was shown at ASDEX why plasmas in
this state can confine energy twice as well as in the L-mode. "A very
effective insulating layer forms at the outer edge of the plasma," Prof.
Wolfrum explained. "The temperature difference between its outside and
the side facing the plasma interior is several million degrees Celsius."
However, the physicists also discovered an unpleasant side effect of
the H-mode: violent energy flares – called edge localised modes (ELMs) –
occur at the plasma edge at regular intervals. "In ASDEX Upgrade, ELMs
are tolerable, but in the much larger ITER they would be so strong that
they would melt the wall of the vacuum vessel," Prof. Wolfrum said. ITER
is being built with four times the vessel radius of ASDEX Upgrade,
which would probably result in ELM energies ten to 15 times as strong as
in ASDEX Upgrade. Therefore, suppression of these perturbations is one
of the most important areas of research in fusion physics. Central
questions concerning H-mode are still unanswered 40 years after its
discovery. For example: How exactly can the transition from L-mode to
H-mode be explained physically? Or: How thick is the insulation layer,
the edge transport barrier? There is still no numerical model that can
completely represent the H-mode. So far, theorists have to feed their
computer codes with certain initial assumptions to calculate individual
phenomena of the H-mode. What they have not yet succeeded in doing is
programming a model in which the transition from L-mode to H-mode
follows quasi inevitably from physics. With such a model, it would then
also be possible to predict the accessibility of the H-mode and the
parameters of the ELMs in the not yet completed ITER experiment. In search of the perfect numerical model This
perfect code would have to combine three physical approaches to
plasmas: neoclassical transport, magnetohydrodynamics (see explanations
below) and turbulence-focused models. Current codes tend to focus on one
of these approaches and, even with this simplification, often keep the
world's best supercomputers busy for months answering limited questions.
But the models are getting better and the computers are getting faster. Two
numerical, non-linear models in particular are in use at IPP, both of
which are being further developed by international teams with IPP's
participation: JOREK is based on the magnetohydrodynamic equations. GENE focuses on micro-turbulences in plasmas. "Through
the interplay of experiments and computer models, we have learned a lot
in understanding the H-mode in recent years," explains Wolfrum. "The
theorists compare our experimental results with their numerical models,
incorporate necessary physical refinements and thereby in turn obtain
results that point us in the direction of new experiments.
These
also always involve adjusting the parameters of plasma density,
temperature and magnetic field, which ultimately determine the movement
of the particles in the plasma and produce certain modes, i.e. operating
modes. Because measurement technology has improved rapidly over the
last four decades, plasmas can now be measured more precisely than when
the H-mode was discovered, which helps to better describe and understand
the plasma state. What researchers now know: the plasma flows
with different velocities at the edge, and it is these flow shears that
play a decisive role in the formation of the edge transport barrier.
They reduce turbulence at the plasma edge and thus lead to the specific
properties of the H-mode. Strategies for suppressing eruptions at the plasma edge Science
has also recently made great strides in the suppression of large edge
localised modes called Type-I ELMs. There are two promising strategies
against the large energy eruptions: 1. Weak magnetic pertubation fields can completely eliminate ELMs in the best case.
In this method, the otherwise completely axisymmetric magnetic field to
confine the plasma is slightly deformed, which, however, reduces the
energy confinement time by 10 to 20 percent. Since 2011, the IPP has
been researching at ASDEX Upgrade how these pertubation fields must be
placed. This method is particularly effective for low plasma densities
at the edge. the pertubation fields amount to one part per thousand of
the strong toroidal field. 2. The formation of large Type I ELMs can also be prevented by promoting the formation of smaller harmless ELMs.
To do this, the otherwise elliptical shape of the plasma cross-section
is deformed in the direction of a rounded triangle with the help of
magnets. The plasma density at the edge is increased. By selectively
blowing more particles into the plasma from the outside, small plasma
eruptions then occur at the edge several thousand times per second,
which are so benign that they cannot endanger the vessel wall. "Through
H-mode research, we are getting closer and closer to plasma operating
states that are most suitable for large fusion facilities like ITER,"
Prof. Elisabeth Wolfrum summarised. The now emeritus H-mode discoverer
Prof. Friedrich Wagner is excited about the completely new possibilities
that the fusion facility in southern France will offer once it is
completed: "ITER will be an instrument like we've never had on Earth
before." From his work on ASDEX – and especially from the H-mode year
1982 – he has learned one thing: "Progress does not always develop
linearly. In between, there are completely unexpected big leaps forward.
That's what makes science so exciting." More Information: https://www.ipp.mpg.de/5280411/05_22
The original publication from 1982: DOI: https://doi.org/10.1103/PhysRevLett.49.1408
Background information: Neoclassical
transport models: the charged particles in a plasma collide with each
other, so that they are deflected from the paths to which, in the
undisturbed state, the applied magnetic fields would force them. The
specially shaped fields in tokamaks typically result in banana-shaped
paths. Numerical models on this basis calculate the path of individual
particles and, collectively, the heat losses from the plasma. Magnetohydrodynamics:
In this research field, the interaction of the applied magnetic field
with electric fields of the particles in the plasma is calculated using a
macroscopic approach. Instead of looking at individual orbits, the
focus here is on average values. The plasma is viewed more or less like a
fluid.
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