Cosmic Plasma, Chapter One: A Survey of the Field
A Professor's Lecture on Hannes Alfvén's Opening Chapter
Good morning, everyone. Today we're going to walk through the first chapter of Hannes Alfvén's remarkable book, Cosmic Plasma. Now, Alfvén won the Nobel Prize in Physics in nineteen seventy, and this book represents the culmination of decades of work trying to understand what most of our universe is actually made of.
Here's the thing most people don't realize: more than ninety-nine percent of the visible matter in the universe exists as plasma. That's the stuff stars are made of, what fills the space between planets, what lights up neon signs, and what we're trying to tame in fusion reactors. And yet, for much of the twentieth century, we got the physics of plasma badly wrong.
That's what this first chapter is about: the story of how we got it wrong, why we got it wrong, and how we might finally start getting it right.
Part One: Two Parallel Roads That Never Met
Alfvén opens by describing something fascinating. Plasma physics developed along two completely separate paths that, for most of history, barely spoke to each other.
The first path was experimental. Starting about a hundred years before Alfvén wrote this book, scientists were studying what they called electrical discharges in gases. You know what this looks like. Lightning bolts. Neon tubes. The glow you see when electricity arcs through air. These experimenters were practical people. They built devices, watched what happened, and tried to describe what they saw.
And what did they see? Frankly, a mess. The plasma did strange things. It would form striations, which are bands of light and dark. It would create double layers, which are thin regions where the electric field suddenly becomes very strong. It would oscillate in complicated ways. Sometimes the electrons would be ten or a hundred times hotter than the surrounding gas. The ions would be somewhere in between.
This was awkward physics. Complicated. Not pretty. Most theoretical physicists looked down on this field because it didn't lend itself to elegant mathematics.
The second path was theoretical. These scientists came from the highly developed study of ordinary gases. They thought, well, a plasma is just an ionized gas, isn't it? We already understand gases very well. Surely we just need to extend our existing theories a little bit to include the electromagnetic forces.
These theories were mathematically beautiful. They claimed to derive everything about plasmas from fundamental principles. But here's the problem: because the mathematics was so complex, the theorists had to make approximations, and those approximations often threw out exactly the complicated phenomena that the experimenters were actually seeing.
The two groups essentially ignored each other.
Part Two: Birkeland's Terrella and the Road Not Taken
Now, there was one person who tried to bridge this gap very early on. His name was Kristian Birkeland, a Norwegian scientist working around nineteen oh eight.
Birkeland did something remarkable. He looked at the aurora, the northern lights, and he looked at magnetic storms, and he wondered: can I recreate these in my laboratory? So he built what he called a terrella, which is just a fancy word for a small magnetized sphere, like a tiny model Earth. He immersed this terrella in a plasma and watched what happened.
And what happened was extraordinary. Under certain conditions, glowing rings appeared around the poles of his little model Earth. Birkeland immediately recognized that these rings looked like the auroral zones, the regions where the northern and southern lights appear on our real planet.
He was right. We now know this is essentially correct.
Birkeland also proposed that the electrical currents causing the aurora must close through vertical paths, flowing along the magnetic field lines. This too was correct, at least as a first approximation.
But here's the tragedy. Birkeland's experimental approach was overwhelmed by the purely theoretical approach. A competing theory, developed by Chapman and Ferraro, became dominant. It was mathematically elegant but had almost no contact with laboratory plasma experiments.
For thirty or forty years, Birkeland's results were forgotten. Textbooks ignored him. Anyone who tried to revive his ideas was dismissed.
Part Three: The Thermonuclear Crisis
The theoretical approach crushed the experimental approach. But only until the theories had to make predictions that could actually be tested.
Here's what happened. From the beautiful theories, scientists concluded that plasma should be easy to confine in magnetic fields. They thought they could heat plasma to enormous temperatures and achieve controlled thermonuclear fusion. This would solve the world's energy problems.
So they built the reactors. And they discovered something shocking.
The plasma didn't believe in the theories.
Alfvén uses exactly this phrase, and I think it's wonderful. The plasma refused to behave the way the elegant mathematics said it should. Instead, it displayed all sorts of complicated effects that the theories had simply ignored. The plasma would escape from its magnetic confinement in unexpected ways. It would develop instabilities the theories hadn't predicted.
This was the thermonuclear crisis. It forced plasma physicists to go back to basics and develop new theories, but this time in close contact with what the plasma actually did in experiments.
But here's the strange thing. This crisis didn't affect cosmic plasma physics very much. The theorists working on space plasmas just kept going with their elegant but disconnected theories. Why? Because for a long time, there was no way to check whether their theories matched reality in space. You couldn't fly up to the magnetosphere and measure things directly.
So speculative theories grew into what Alfvén calls a gigantic structure, built entirely on a foundation that laboratory experiments had already proven was false.
Part Four: When Spacecraft Met Reality
Then came the space age. Suddenly we could actually send instruments into the magnetosphere and measure what was happening.
The first results seemed to match the accepted theories, or could at least be interpreted that way. But as measurement techniques improved, the discrepancies became impossible to ignore.
Alfvén includes a wonderful figure showing how our understanding of the space around Earth changed between the nineteen fifties and the nineteen seventies. In the fifties, scientists assumed the Earth was surrounded by vacuum and that its magnetic field extended outward in a simple, undisturbed pattern. By the sixties, we knew about the Van Allen radiation belts, the bow shock where the solar wind slams into our magnetic field, the magnetopause boundary, and the long magnetic tail stretching away from the Sun. By the seventies, the picture had become far more complex, with intricate current systems that the original theories had never anticipated.
The plasma in space turned out to be just as complicated as the plasma in laboratory discharge tubes. It followed the same basic laws, not the idealized laws of the elegant theories.
Part Five: The Scaling Problem
This brings us to one of the central challenges in cosmic plasma physics: the problem of scale.
In a laboratory, plasma experiments might be about a tenth of a meter across. The Earth's magnetosphere is about ten million meters across. The heliosphere, the bubble of solar wind that surrounds our entire solar system, is billions of meters across. And galactic phenomena are larger still, by another factor of a billion or more.
So when we observe something in a laboratory plasma, how do we know the same physics applies to a plasma a billion billion times larger?
This is the scaling problem. Different plasma parameters scale in different ways, and translating results from one regime to another requires deep understanding of which features are universal and which depend on size.
Alfvén distinguishes between two types of simulation experiments that help with this.
The first is pattern simulation. You build an apparatus that geometrically resembles the cosmic situation. Birkeland's terrella was exactly this kind of experiment. You create a small model and see if it behaves like the larger system.
The second is process simulation. Here you don't try to recreate the whole geometry. Instead, you study the fundamental behaviors of plasma in the laboratory. You learn what plasma actually does under various conditions. This builds the theoretical foundation that you then apply to cosmic situations.
Computer simulation is also valuable, Alfvén says, but it can never replace process simulation. The computer can only calculate what you tell it to calculate. If you don't know the basic properties of plasma from real experiments, you can't program them correctly. As Alfvén puts it, the computer is not a good physicist if its programmer is not.
Part Six: The Essential Dualism
Now we come to what I think is the most important idea in this chapter, and really the central theme of the entire book.
In plasma physics, there are two ways to describe what's happening. You can describe magnetic fields, or you can describe electric currents. Mathematically, these are equivalent. If you know one, you can calculate the other. But conceptually and practically, they are very different.
Measuring magnetic fields in space is relatively easy. Put a magnetometer on a spacecraft and you can measure the field directly. Measuring electric currents is much harder, sometimes impossible. So naturally, space scientists present their results in terms of magnetic field configurations.
Furthermore, in the mathematical theory called magnetohydrodynamics, it's convenient to eliminate the electric current from your equations and represent everything in terms of the magnetic field. This approach works fine for many phenomena.
But there are other phenomena that absolutely require you to think explicitly about the electric current. If you try to understand them using only the magnetic field picture, you will get the wrong answer.
What kinds of phenomena require the current picture? Alfvén gives us a list.
First, energy transfer from one region to another. When energy moves through a plasma, it's carried by currents, and you need to trace those currents to understand where the energy goes.
Second, the formation of double layers. These are thin regions where the electric field suddenly becomes very strong, and particles crossing them get accelerated to high energies. You cannot understand double layers without thinking about currents explicitly.
Third, explosive events. Solar flares, magnetic substorms in Earth's magnetosphere, stellar flares. These all involve sudden releases of energy, and they occur when currents are disrupted. The magnetic field picture alone cannot explain how energy gets concentrated so rapidly at a single point.
Fourth, there's something called the Ferraro corotation violation. In certain situations, plasma doesn't rotate with a magnetized body the way simple theory predicts. Double layers can create what Alfvén calls partial corotation, and this turns out to be essential for understanding how our solar system formed.
Fifth, the formation of filaments. Plasma loves to organize itself into thin threads of current. You see this in the aurora, in the solar atmosphere, in nebulae. The magnetic field picture doesn't predict this. The current picture does.
Sixth, the cellular structure of space. Current sheets form boundaries that divide space into cells. This gives the cosmos a fundamentally different character than a smooth, homogeneous medium.
Alfvén summarizes this with a striking diagram. Some phenomena belong to the magnetic field picture. Some belong to the electric current picture. Trying to analyze phenomena with the wrong picture leads to errors. The two approaches are complementary, like the wave and particle pictures of light.
Part Seven: What We Can and Cannot Know
Alfvén draws a very important line in this chapter. He distinguishes between regions of space where we can actually send instruments and measure things directly, and regions so far away that we can only observe them from a distance.
In the regions we can reach, primarily Earth's magnetosphere and the nearby parts of the heliosphere, we can do real science. We can test our theories against measurements. We can discriminate between competing interpretations.
In the distant regions, everything is necessarily more speculative. We can apply our best understanding of plasma physics, but we cannot be certain we've got it right.
This is crucially important for cosmology, the study of the universe as a whole. Much of cosmology deals with regions we will never visit. The only way to approach these problems responsibly, Alfvén argues, is to first thoroughly understand plasma in the regions we can actually test. Then, with that firm empirical foundation, we can cautiously extend our understanding outward.
This is the opposite of what much of twentieth century cosmology did. Too often, theorists developed speculative models for distant regions without first checking whether their basic assumptions worked in the places we could actually measure.
Part Eight: The Aims of This Book
Alfvén closes the chapter by stating his goals for the entire book.
First, he wants to systematically compare different regions of plasma. From laboratory scale to planetary magnetospheres to galactic dimensions, he wants to understand what's universal and what changes with scale.
Second, he wants to supplement the traditional magnetic field description with an explicit electric current description. Both pictures are needed. Both must be used together.
Third, he wants to maintain a strict distinction between what we know and what we're guessing. Regions accessible to measurement are one thing. Distant regions are necessarily speculative, and we should be honest about that.
There's also an unstated aim that pervades the whole book. Alfvén wants to rehabilitate the experimental approach that was nearly killed off in the early twentieth century. He wants to reconnect plasma physics to laboratory reality. He wants to end the reign of beautiful but disconnected theories.
Closing Thoughts
What makes this chapter so remarkable is its combination of scientific rigor and historical honesty. Alfvén doesn't pretend that physics progresses smoothly from one correct theory to another. He shows us the wrong turns, the dogmas, the resistance to new ideas.
Science, he's telling us, is not just a collection of facts. It's a human activity, subject to fashion and prejudice and the politics of funding. Sometimes the right ideas get buried. Sometimes beautiful mathematics leads us astray. The only reliable guide is nature itself, the plasma that refuses to believe in theories that don't match what it actually does.
In the chapters that follow, Alfvén will build up a picture of cosmic plasma that's rooted in laboratory experiments and space measurements. He'll show us electric circuits spanning millions of kilometers. He'll show us how energy flows through the cosmos. He'll show us a universe that's far more complex and interesting than the smooth, featureless models that dominated for too long.
But all of that starts here, with this honest accounting of where we went wrong and what it will take to get things right.
That's Chapter One. Any questions before we move on?