Principles of Radiation Physics Part 1: X-Ray Production
Nov 18, 2025

If you want to become a radiologic technologist who operates with confidence and calm, you must first understand the world that exists inside the x-ray tube. Not the buttons on the console, not the motions of positioning—but the invisible process that creates the very thing you work with every day: the x-ray beam.
Most students see physics as something distant, abstract, or overly technical. But physics is not distant. It is the foundation beneath every exposure you make. It is the structure that supports your judgment, your technique, and ultimately your patient’s safety.
There’s a discipline to understanding x-ray production—an anchor-like steadiness that helps you think clearly instead of guessing. And if you want to reach your full potential as a radiologic technologist, this clarity is not optional. It’s essential.
Your uploaded documents describe four fundamental steps in the creation of x-rays:
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A source of free electrons
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Acceleration of electrons
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Focusing of electrons
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Deceleration of electrons
Everything in diagnostic imaging begins here. So let’s walk through these steps—not quickly, not superficially, but slowly enough that the logic becomes second nature.
1. The Source of Free Electrons: Thermionic Emission
Inside the x-ray tube, at the cathode, sits a tungsten filament. When electrical current passes through this filament, it heats up. And as the temperature increases, electrons gain enough energy to break free from the metal.
Your documents call this thermionic emission.
The filament “boils” electrons off its surface, forming what the lecture transcript describes as a space charge—a cloud of free electrons gathered near the filament.
This cloud is where every x-ray begins.
But electrons do not leave the filament in random bursts. Their release depends on:
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The filament current
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The temperature of the filament
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The space charge effect, which limits how many electrons can accumulate
Understanding this step teaches you something simple yet vital:
Nothing in the x-ray tube happens by accident. Everything is controlled, intentional, and governed by physical law.
2. Acceleration of Electrons: The Role of kVp
Once the electrons are freed, they must be accelerated with enormous force toward the anode.
This is where kilovolt peak (kVp) enters the picture.
The kVp applied across the tube creates a powerful electrical potential difference. This potential pulls electrons from the negatively charged cathode across a vacuum toward the positively charged anode.
Your uploaded documents emphasize:
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Higher kVp = higher electron speed
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Higher electron speed = higher energy photons
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Higher kVp increases both beam quality and penetration
Electrons accelerated across the tube reach speeds approaching half the speed of light. That speed is not a metaphor—it is real velocity, real power.
And yet the process remains orderly. Purposeful. Predictable.
Physics teaches a lesson here: power is meaningless without direction. Electron velocity only matters if it can be applied with precision. That precision comes in the next step.
3. Focusing of Electrons: The Focusing Cup
Free electrons must be directed; otherwise, they scatter.
The cathode assembly contains a focusing cup, a negatively charged metal structure shaped to steer the electron cloud into a narrow stream. This stream is aimed at the small target area on the anode.
Your documents note that without the focusing cup:
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Electrons would spread out
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Image sharpness would diminish
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Heat loading would become dangerously uneven
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Tube efficiency would drop
The focusing cup imposes order. It channels potential into purpose.
This is where the process becomes elegant. Something chaotic—a cloud of electrons—becomes a tight, precise beam. And that beam is ready for the final step.
4. Deceleration: The Moment X-Rays Are Born
Electrons traveling at high velocity collide with the tungsten target of the anode and undergo sudden deceleration.
This moment—the collision, the stop, the loss of speed—is where x-rays are created.
Your documents outline two results of this impact:
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Bremsstrahlung radiation
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Characteristic radiation
This is where the electron’s kinetic energy is converted into electromagnetic energy.
This is where physics becomes imaging.
This is where the x-ray beam takes shape.
More than 99% of the interaction becomes heat. Less than 1% becomes usable x-ray photons. Yet that tiny fraction is powerful enough to reveal anatomy, detect disease, and guide treatment.
This is the paradox of x-ray production:
Almost all the energy becomes something you cannot use.
But the small part you can use changes everything.
Once electrons collide with the tungsten target inside the anode, the process shifts. Up to that point, everything is motion—electrons released, accelerated, focused. But here, in the last fraction of a millimeter, motion becomes energy. Collisions become information. Physics becomes the image.
Your uploaded documents define two interactions that create diagnostic x-rays:
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Bremsstrahlung radiation
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Characteristic radiation
To understand these well is to understand the beam itself.
Bremsstrahlung Radiation: The Backbone of the X-Ray Beam
Bremsstrahlung radiation—often shortened to “Brems”—is the primary component of the diagnostic x-ray spectrum. Your documents make this clear: it accounts for the vast majority of the photons in the beam.
Here’s how it works:
A high-speed electron from the cathode approaches the positively charged tungsten nucleus. It does not have to strike the nucleus directly. The nucleus’s strong positive field pulls on the electron as it passes, causing it to slow down or change direction. This deceleration forces the electron to release energy in the form of an x-ray photon.
The characteristics of Brems radiation according to your materials:
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It produces a wide range of energies
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It creates a continuous spectrum
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Its maximum energy is controlled by the kVp you set
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It is the dominant form of x-rays used in imaging
This interaction is sensitive to your technique:
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Raise kVp → increase both photon energy and number of photons
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Lower kVp → decrease beam quality and penetration
Bremsstrahlung is flexible, adaptive, and abundant. It is the foundation of diagnostic x-ray production.
Characteristic Radiation: A Discrete, Predictable Signature
Where Bremsstrahlung is broad and varied, characteristic radiation is precise.
Your documents describe the process:
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A high-speed electron strikes a K-shell electron of the tungsten atom.
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It ejects that K-shell electron, creating a vacancy.
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An electron from a higher shell (L, M, or N) drops down to fill the gap.
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This transition releases energy as an x-ray photon.
Because tungsten’s K-shell binding energy is 69.5 keV, a K-shell characteristic photon must have at least that much energy.
That means:
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Characteristic radiation has fixed energy levels
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It forms sharp, discrete spikes on the emission spectrum
In diagnostic imaging, characteristic radiation from tungsten only appears when the tube operates at 70 kVp or higher, because the incident electrons must be energetic enough to remove K-shell electrons.
Characteristic photons are fewer in number, but they are structurally important. They demonstrate that the beam is not random—its energies reflect the atomic structure of tungsten.
The Line-Focus Principle: Managing Heat While Preserving Detail
Your documents emphasize that the anode must solve a physical problem:
How do you produce a sharp image while absorbing the heat of thousands of electron collisions every second?
The answer is the line-focus principle.
The anode is angled—commonly around 12°. This creates:
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A large actual focal spot, which spreads out heat
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A small effective focal spot, which improves resolution
This design allows the tube to withstand high heat loads without sacrificing detail.
The actual focal spot is the real area the electrons hit.
The effective focal spot is the area projected down onto the patient.
This principle is why images remain sharp even during heavy technique use.
The Anode Heel Effect: Intensity Is Not Equal Across the Beam
Your uploaded documents also describe the anode heel effect, a consequence of the angled anode.
Because x-rays on the anode side must pass through more of the target material:
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The anode side of the beam is less intense
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The cathode side of the beam is more intense
This matters clinically:
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Place the thicker anatomy under the cathode
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Place the thinner anatomy under the anode
Examples given in your materials include:
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Chest: cathode over diaphragm
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Femur: cathode over proximal end
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T-spine: cathode over lower spine
The heel effect is not a flaw.
It is a tool.
A radiographer who uses it intentionally produces better exposures with more consistent penetration.
The deeper you go into x-ray physics, the more you realize something:
This isn’t just science.
It’s a framework for thinking.
Your documents describe the mechanics and mathematics of x-ray production. But beneath the formulas is something more important for your life as a radiographer—a way of approaching your work with clarity instead of guesswork.
Once you understand how x-rays are produced, you stop memorizing techniques and start reasoning through them. You stop being a button-pusher and start becoming a professional.
Let’s bring this chapter together by examining what this knowledge means for you—the radiography student, the future technologist, the person preparing for the ARRT® exam.
1. X-Ray Production Determines the Quality of Every Image
You cannot separate a diagnostic image from the physical process that produced it.
Everything rests on:
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how many electrons were boiled off
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how fast they were accelerated
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how well they were focused
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how they interacted with the tungsten target
Your uploaded documents emphasize that kVp controls beam quality.
It determines:
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the energy of Brems photons
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the presence of characteristic photons (only above 70 kVp)
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the beam’s ability to penetrate anatomy
This means:
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Too little kVp → underpenetration, excessive contrast, noise
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Too much kVp → overpenetration, long grayscale, loss of detail
Technique charts make sense when you understand x-ray production. They are not arbitrary—they are physics applied to anatomy.
Radiographers who understand this do not guess.
They select exposure factors with intention.
2. Heat Management Is Not Optional—It’s Science
Your materials repeatedly highlight a truth students often underestimate:
99% of the energy inside the tube becomes heat.
Only about 1% becomes x-rays.
This imbalance means radiographers must respect:
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heat units
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tube cooling charts
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anode rotation
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exposure timing
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limits on repeated exposures
The tungsten target, the anode angle, the rotating design—every part of the tube is built to manage heat.
Ignoring tube heat doesn’t merely risk equipment damage—
it risks delaying patient care when the tube fails.
Your understanding of this is part of your professionalism.
3. The Focal Spot Is the Gatekeeper of Resolution
Your uploaded documents explain the role of the focusing cup, the actual focal spot, and the effective focal spot. These determine how sharp your images are.
A smaller effective focal spot means:
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better spatial resolution
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clearer edges
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sharper fine detail
But it also means:
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less heat capacity
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greater stress on the anode
This is why high-detail imaging (like extremities or small bones) uses a small focal spot, while high-heat techniques (like abdomen or portable chest) require a large one.
A radiographer who understands focal spot physics doesn’t choose out of habit—they choose out of knowledge.
4. Clinical Positioning Is Influenced by the Anode Heel Effect
The heel effect becomes a clinical tool once you understand it:
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The cathode side is more intense
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The anode side is less intense
Your documents instruct you to apply this to patient care:
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Thicker anatomy → cathode
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Thinner anatomy → anode
This is not a trick.
It is not a shortcut.
It is physics shaping better patient outcomes.
Using the heel effect is part of becoming a technologist who thinks rather than imitates.
5. Understanding the Spectrum Helps You Predict Contrast
Bremsstrahlung radiation creates a broad spectrum of energies.
Characteristic radiation adds discrete peaks above 69.5 keV.
These two components interact with tissue differently:
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Higher-energy photons penetrate more
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Lower-energy photons contribute to subject contrast
This means your chosen kVp changes not only penetration but the tonal structure of the final image.
When you understand x-ray production, you understand why:
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chest x-rays use high kVp
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extremities use low kVp
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spine uses moderate kVp
Technique becomes a language you can speak, not a list you memorize.
6. X-Ray Production Shapes Dose and Safety
Nothing in your documents is more central to patient care than this principle:
Radiation dose cannot be managed if the beam is not understood.
Because kVp affects photon energy, and mAs affects beam quantity:
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Choosing the correct kVp reduces unnecessary dose
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Using the right mAs prevents repeats
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Using a proper focal spot protects the tube
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Understanding heat limits prevents equipment failure
Your comprehension of x-ray production influences ALARA more than any other concept in physics.
7. Closing Reflection: The Radiographer Who Understands the Nature of the Beam
Physics will never ask for your admiration.
It will not demand your excitement.
It quietly asks for your respect—and rewards you with mastery.
X-ray production is not something you cram the night before the exam. It is a set of principles that shape:
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the quality of your images
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the confidence behind your decisions
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the safety of your patients
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the longevity of your equipment
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the clarity of your thinking
When you understand the process inside the tube, you work differently.
You think differently.
You carry yourself differently.
You move from uncertainty to competence.
From memorization to understanding.
From student to technologist.
This is the foundation.
This is where excellence begins.
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