Basic Guide to Dental Radiography (eBook)
John Wiley & Sons (Verlag)
978-1-118-91627-8 (ISBN)
- Comprehensive coverage includes general physics, principles of image formation, digital image recording, equipment, biological effects of x-rays and legislation
- Suitable for the whole dental team
- Illustrated in full colour throughout
- Ideal for those completing mandatory CPD in radiography
- Useful study guide for the NEBDN Certificate in Dental Radiography, the National Certificate in Radiography or the Level 3 Diploma in Dental Nursing
Tim Reynolds has worked for many years as a radiographer in the NHS. Outside of clinical work Tim has worked in radiographic education for more than 20 years. Tim was a nationally elected member of the College of Radiographers Council. During his time on Council he was a member of the team that liaised with the Dental Nurse Standards Advisory Board to jointly develop the syllabus of study which provided the model for dental nurse radiography courses. He also sat on the National Executive of the British Radiation Protection Association. Formerly Principal Tutor for the Diagnostic Radiography undergraduate course at Keele University, Tim now runs his own educational consultancy specialising in radiography training for dental nurses.
Basic Guide to Dental Radiography provides an essential introduction to radiography in the dental practice. Illustrated throughout, this guide outlines and explains each topic in a clear and accessible style. Comprehensive coverage includes general physics, principles of image formation, digital image recording, equipment, biological effects of x-rays and legislation Suitable for the whole dental team Illustrated in full colour throughout Ideal for those completing mandatory CPD in radiography Useful study guide for the NEBDN Certificate in Dental Radiography, the National Certificate in Radiography or the Level 3 Diploma in Dental Nursing
Tim Reynolds has worked for many years as a radiographer in the NHS. Outside of clinical work Tim has worked in radiographic education for more than 20 years. Tim was a nationally elected member of the College of Radiographers Council. During his time on Council he was a member of the team that liaised with the Dental Nurse Standards Advisory Board to jointly develop the syllabus of study which provided the model for dental nurse radiography courses. He also sat on the National Executive of the British Radiation Protection Association. Formerly Principal Tutor for the Diagnostic Radiography undergraduate course at Keele University, Tim now runs his own educational consultancy specialising in radiography training for dental nurses.
Acknowledgements viii
1 General physics 1
2 X?-ray production 12
3 X?-ray interaction with matter 27
4 Principles of image formation 36
5 Imaging with dental X?-ray film 46
6 Digital imaging recording 61
7 X?-ray equipment 70
8 Radiation doses and dose measurement 78
9 Biological effects of X?-rays 86
10 Legislation: Ionising Radiations Regulations 1999 (IRR 1999) 94
11 Legislation: Ionising Radiation (Medical Exposures) Regulations 2000 (IR(ME)R 2000), Statutory Instrument 1059 108
12 Quality assurance 114
13 Dental intra?-oral paralleling techniques 128
14 Orthopantomography 159
15 Other dental radiographic techniques 170
Appendix A: Adequate training 189
Appendix B: Image quality troubleshooting 192
Index 201
Chapter 1
General physics
ATOMS AND MOLECULES
Whenever setting out on a project of this type, it is difficult to know what to use as your starting point.
Let us start by looking at what makes up the world as we know it.
We look around and see lakes, mountains, fields, etc., but what if we could look into these things and see what makes them what they are?
We would see atoms and molecules.
There can’t be many people who have not heard of these, but what are they?
Atoms and molecules are linked to elements and compounds (here is the problem – almost every time we mention anything, it will lead us straight to something else we need to know).
Elements are single chemical substances such as oxygen, hydrogen, sulphur, etc. We can take a large amount of an element and keep cutting it down to make it smaller and smaller, but there is a limit to how small we can make it.
We come to a point where all that we have is a single atom of the substance; if we then cut it to an even smaller size, we will be breaking down the atom, and it will no longer be that particular substance.
- Atoms are the smallest particle of an element that can exist and still behave as that element.
Breaking down an atom eventually produces just a collection of the bits that make up the atom.
Here we go again! What is smaller than an atom? Or what are atoms made of?
There are many so‐called fundamental particles that make up the atoms that provide the basic building blocks for all of the things that we see, touch and know of. Some of these fundamental particles are only now being discovered.
For the purposes of fulfilling the basic guide brief, we will concentrate on only three types of particle: protons, neutrons and electrons.
Protons and neutrons are large (that’s relative; remember we would need very powerful microscope to see even these particles), and electrons are small.
To represent the difference in these particles in a way you can visualise, think of placing a single grape pip on the ground and then standing a person 6 ft tall next to it.
The grape pip represents the size of an electron, and the 6‐ft‐tall person the size of a proton or a neutron. Protons and neutrons are slightly different in size, but for our purposes they can be considered to be the same, but electrons are 1840 times smaller than either of the other two particles.
The protons and electrons each have an electrical charge and these charges are of opposite poles (like the two ends of a battery). The protons have a positive charge (+ve), and the electrons a negative charge (−ve).
Despite the relative size difference of the particles, the two charges, although opposite poles (or signs), are of equal size or strength.
So the positive charge on one large proton is completely cancelled out by the negative charge on one tiny electron.
Neutrons have no charge at all (they are neutral).
How do these particles fit together to make an atom?
Figure 1.1 shows what has become an accepted idea of the appearance of an atom.
Figure 1.1 Classic basic model for the structure of the atom
There is a large central nucleus, containing protons and neutrons with the electrons circling in a number of orbits at different distances from the nucleus. These orbits have traditionally been called electron shells or energy shells.
This model will be adequate for our understanding, but do remember that the electron orbits are not all in the same plane. The atom is three‐dimensional, and the electron orbits taken all together would make a pattern much more like looking at a football.
This makes sense if you think of the electron orbits as actual shells; they completely surround the nucleus much like the layers of an onion. This is difficult to demonstrate on a flat page, and we have become used to the picture as shown (Figure 1.1) with lots of circles having the same centre.
The number of protons in the nucleus tells us what sort of atom it is. A nucleus containing 6 protons would be a carbon nucleus, 11 protons sodium, and 82 protons lead. The number of protons present is the atomic number of the element and of course of the atom; the number of protons in fact tells us what chemical substance the atom is.
The protons in the nucleus all have a positive charge, and the tendency for positive charges is to push each other apart just like two magnetic north or two south poles would. They need something to keep them from pushing each other away; this function is performed by the neutrons. The neutrons don’t do this job alone, but for the purposes of this particular text, we need look no further into nuclear forces. At very low atomic numbers, there will be equal numbers of protons and neutrons; however as atomic number increases, the higher concentration of positively charged protons needs a higher number of neutrons to overcome the forces of repulsion between them.
The number of electrons in each orbit is specific and is determined by the following formula:
where E is the number of electrons and n is the number of the electron shell.
So, the closest shell to the nucleus is number 1. In that shell, you can have 2 × 12 electrons.
12 is 1 × 1 so that 1 multiplied by 2 tells us we can have two electrons in the first shell.
In the second shell we can have 2 × 22. So 2 × 2 (n2) = 4 multiplied by 2 gives 8.
In the third shell 2 × 32 gives 2 × 9. So 18 electrons would be allowed in shell 3.
No electrons can be positioned in shell 2 if shell 1 is not full and none in shell 3 if shell 2 is not full. That is to say that all inner shells must be filled before outer shells can contain any electrons. If an electron were removed from an inner shell, then one would move down from an outer shell to fill the gap. (This becomes important when we consider the effects of exposure to radiation.)
The process works like this because atoms always exist in their lowest energy state (ground state) and inner shell electrons are the low energy ones. So if we take out a low‐energy inner shell electron, the atom is at a higher level of energy than it could be, so an electron from a shell further out falls to fill the gap and in the process gives up some of its energy.
The electron filling the gap will give up some energy because it can only be in the lower shell if it has the correct level of energy. This process will continue until the exchange takes place at the outermost shell of the atom. There will then be an electron space free in the outer shell of the atom (the one that is the greatest distance from the nucleus) (Figure 1.2).
Figure 1.2 Redistribution of electrons to the atoms’ lowest energy state
From the previous descriptions, it is clear that most of the mass of an atom (it’s easier to think of this as weight or just the solid material) is in the nucleus of the atom.
A carbon atom with 6 protons and 6 neutrons (there are forms of carbon with a different number of neutrons, but we are not concerned with isotopes in this text) will have 6 electrons circulating in two discrete orbits (2 in shell 1 and 4 in shell 2). So in terms of the sheer bulk of material in relative terms, the electrons account for six times one, and the nucleus for 12 times 1840.
This means the solid matter that makes up an atom is mostly contained in the nucleus (where the big particles are). However if we look at the overall size of the atom (from one side of the outer electron shell to the other), most of it is not made up of material at all but of empty space. Even taking into account the relatively large particles in the nucleus, all elements including things like lead have atoms that are almost entirely free space. This is sort of like a large fishing net on a trawler; if the net was 50 yd by 50 yd, the overall size is massive, but if you just put the material making the net together, it would be tiny by comparison; the overall measurements of the net are made up mostly of the gaps between the materials.
To round off our investigation of atoms, the following is presented.
The electron shells are not called 1, 2 and 3 but are denoted by letters, number 1 is K, number 2 L, number 3 M, and so on; this form of atomic structure will be found in any basic science or physics book though not in advanced texts on the topic. The shell numbers simply allow us to calculate the number of electrons allowed to be in the particular orbit or shell.
On page 1 when we started talking about atoms, we also mentioned molecules, so we now need to bring those back into our thinking.
When we introduced molecules we said the atoms and molecules were linked to elements and compounds.
We have discussed elements, so what are compounds?
A compound is a combination of two or more elements; a combination that everyone knows is H2O (water).
The formula indicates that there are two hydrogen atoms and one of oxygen. The collection of three atoms shown is a molecule of water. If we try to cut this down to make an even smaller amount, we end up with something that is no longer water. Take the oxygen out and we simply have two atoms of hydrogen; if we take away an hydrogen atom, we have an hydroxide or an hydroxyl...
| Erscheint lt. Verlag | 22.8.2016 |
|---|---|
| Reihe/Serie | Basic Guide Dentistry Series |
| Basic Guide Dentistry Series | Basic Guide Dentistry Series |
| Sprache | englisch |
| Themenwelt | Medizin / Pharmazie ► Allgemeines / Lexika |
| Medizin / Pharmazie ► Gesundheitsfachberufe | |
| Medizin / Pharmazie ► Medizinische Fachgebiete ► Radiologie / Bildgebende Verfahren | |
| Medizin / Pharmazie ► Zahnmedizin | |
| Schlagworte | basic guide to • CPD radiography • Dental Hygiene & Therapy • dental nurse • Dental Nursing • Dental Radiography • Dental Team • dentistry • Gesundheits- u. Sozialwesen • Health & Social Care • Praxis der Zahnarzthelferin • Radiographie • radiography • Zahn • Zahnmedizin • Zahn- u. Mundhygiene u. Therapie |
| ISBN-10 | 1-118-91627-1 / 1118916271 |
| ISBN-13 | 978-1-118-91627-8 / 9781118916278 |
| Informationen gemäß Produktsicherheitsverordnung (GPSR) | |
| Haben Sie eine Frage zum Produkt? |
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