RADIATION MEASUREMENTS AND MONITORING.pptx

AbubakarHammadama 32 views 32 slides Aug 08, 2024
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About This Presentation

radiation measurement


Slide Content

RADIATION MEASUREMENTS AND MONITORING By Prof Kabiru Isyaku Radiology Department, Bayero University Kano

Measuring RadiationMeasuring Radiation There are basically three common measurements of radiation The amount of radioactivity Ambient radiation levels Radiation dose. To get accurate and reliable measurements, we need to have both the right instrument and a trained operator. It is important to maintain radiation detection equipment to ensure it is working properly.

When working with radiation, we are concerned about the amount of energy the material is emitting. The size, weight, and volume of the material do not necessarily matter. A small amount of material may give off a lot of radiation. On the other hand, a large amount of radioactive material may give off a small amount of radiation .

For example, imagine we had a jar filled with radioactive material. We want to find out how many radioactive atoms decay every second, giving off alpha particles, beta particles, or gamma rays. This is the amount of radioactivity  in the jar We also want to find out how much of the radiation from the material in the jar actually makes it to any given location. This type of measurement will give us the  ambient radiation levels  at this location . We are especially interested to know how much radiation is absorbed by the body while standing next to this jar i.e. the   radiation dose .

Radiation Dose Radiation dose  is the amount of radiation absorbed by the body. If we know the ambient radiation level, we easily can calculate our radiation dose. Imagine the ambient radiation levels coming from this jar where this person is standing are 0.5 Sv /h. If this person stands in the same place for one hour, he will receive a dose of 0.5 Sieverts. But, if he moves away from the jar, the ambient radiation levels will drop, and so will his dose.  Putting   distance  between yourself and radioactive material is a key principle of radiation safety.

Units for Measuring Radiation Dose Most scientists in the international community measure radiation using the System Internationale (SI), a uniform system of weights and measures that evolved from the metric system. In the United States, however, the conventional system of measurement is still widely used. Different units of measure are used depending on what aspect of radiation is being measured e.g. the amount of radiation being given off, or emitted, by a radioactive material is measured using the conventional unit  curie  (Ci), named for the famed scientist Marie Curie, or the SI unit  becquerel  ( Bq ). The radiation dose absorbed by a person (that is, the amount of energy deposited in human tissue by radiation) is measured using the conventional unit  rad  or the SI unit  gray  ( Gy ). The biological risk of exposure to radiation is measured using the conventional unit  rem  or the SI unit  sievert  ( Sv ).

To report the radiation dose, we use either: The international unit for dose, the Sievert ( Sv ) or the Gray ( Gy ) The United States unit for dose, the rem or the rad It is common to see variations of these units such as: millisievert ( mSv ) millirem ( mrem ) Converting between international units and U.S. units is easy for dose: 1 Sv = 100 rem 1rem = 10 mSv 1 Gy = 100 rad 1 rad = 10 mGy

The average dose we receive every year, just from living on Earth, is approximately 3 mSv . About two-thirds of that dose comes from radon, a gas that occurs naturally from the breakdown of uranium. Medical procedures add another 3 mSv , on average, bringing the total annual exposure for the average person to slightly more than 6 mSv . But, as individuals, the radiation doses we may receive in any one year can vary quite a bit .

There are many things that can influence our radiation dose in any year: Some types of radiation, like natural background radiation, are present all the time and provide a continuous dose that accumulates over time. This natural background depends on a number of factors. For example: If you live at higher elevation, you receive a higher dose of cosmic radiation. If you share a bed with your spouse or partner, you each get a small dose of radiation from the naturally occurring radioactive potassium-40 in each other’s body. You irradiate each other during the night. You may live in a home that has elevated radon levels.

Medical imaging procedures used in diagnostic exams such as x-rays and CT scans provide a one-time dose – you receive the radiation during the test and that’s it. Other medical procedures, such as nuclear medicine, may involve giving you a small amount of radioactive material to assist in imaging. In that case, you will emit radiation for up to several days after the exam. The frequency of activities such as medical procedures that provide one-time doses will impact your annual radiation dose.

This does not mean that medical procedures like CT scans are harmful. The dose you receive from these and other medical procedures comes with a benefit – the imaging helps doctors make a diagnosis. But it is important to consider the risks and benefits of any procedure or activity that exposes you to ionizing radiation.

Measuring Emitted Radiation The unit of emitted radiation is measured in the conventional unit Ci or the SI unit Bq . A radioactive atom gives off or emits radioactivity because the nucleus has too many particles, too much energy, or too much mass to be stable. The nucleus breaks down, or disintegrates, in an attempt to reach a nonradioactive (stable) state. As the nucleus disintegrates, energy is released in the form of radiation. The Ci or Bq is used to express the number of disintegrations of radioactive atoms in a radioactive material over a period of time e.g. one Ci is equal to 37 billion (37 X 10 9 ) disintegrations per second. The Ci is being replaced by the Bq . Since one Bq is equal to one disintegration per second, one Ci is equal to 37 billion (37 X 10 9 ) Bq . Ci or Bq may be used to refer to the amount of radioactive materials released into the environment. For e.g. during the Chernobyl power plant accident that took place in the former Soviet Union, an estimated total of 81 million Ci of radioactive cesium (a type of radioactive material) was released.

Measuring Radiation Dose When a person is exposed to radiation, energy is deposited in the tissues of the body. The amount of energy deposited per unit of weight of human tissue is called the absorbed dose. Absorbed dose is measured using the conventional  rad  or the SI  Gy . The rad, which stands for radiation absorbed dose, was the conventional unit of measurement, but it has been replaced by the  Gy . One Gy is equal to 100 rad.

Measuring Biological Risk A person’s biological risk (that is, the risk that a person will suffer health effects from an exposure to radiation) is measured using the conventional unit  rem  or the SI unit  Sv . To determine a person’s biological risk, scientists have assigned a number to each type of ionizing radiation (alpha and beta particles, gamma rays, and x-rays) depending on that type’s ability to transfer energy to the cells of the body. This number is known as the Quality Factor (Q). When a person is exposed to radiation, scientists can multiply the dose in rad by the quality factor for the type of radiation present and estimate a person’s biological risk in rems. Thus, risk in rem = rad X Q. The rem has been replaced by the Sv . One Sv is equal to 100 rem.

Abbreviations for Radiation Measurements Prefix Equal to How Much Is That? Abbreviation Example atto- 1 X 10 -18 .000000000000000001  a  aCi femto- 1 X 10 -15 .000000000000001  f  fCi pico- 1 X 10 -12 .000000000001  p  pCi nano- 1 X 10 -9 .000000001  n  nCi micro- 1 X 10 -6 .000001  µ  µCi milli- 1 X 10 -3 .001  m  mCi centi- 1 X 10 -2 .01  c   cSv

Abbreviations for Radiation Measurements Table 2 Prefix Equal to How Much Is That? Abbreviation Example kilo- 1 X 10 3 1000  k  kCi mega- 1 X 10 6 1,000,000  M  MCi giga- 1 X 10 9 100,000,000  G  GBq tera- 1 X 10 12 100,000,000,000  T  TBq peta- 1 X 10 15 100,000,000,000,000  P  PBq exa- 1 X 10 18 100,000,000,000,000,000  E   EBq

Common Radiation Exposures Source of exposure Dose in rem Dose in sievert ( Sv ) Exposure to cosmic rays during a roundtrip airplane flight from New York to Los Angeles 3 mrem 0.03 mSv One dental x-ray 5 mrem 0.05 mSv One chest x-ray 10 mrem 0.1 mSv One mammogram 70 mrem 0.7 mSv One year of exposure to natural radiation (from soil, cosmic rays, etc.) 300 mrem 3 mSv

When talking about radiation detection instruments, there are three types of detectors that are most commonly used, depending on the specific needs of the device. These are:  Gas-Filled Detectors Scintillators Solid State detectors .

Gas Filled Detectors The gas-filled detectors, are amongst the most commonly used. There are several types of gas-filled detector, and while they have various differences in how they work, they all are based on similar principles.  When the gas in the detector comes in contact with radiation, it reacts, with the gas becoming ionized and the resulting electronic charge being measured by a meter.   The different types of gas-filled detectors are: ionization chambers, proportional counters, and Geiger-Mueller (G-M) tubes. The major differentiating factor between these different types is the applied voltage across the detector, which determines the type of response that the detector will register from an ionization event.

Ionization chambers These are lower end of the voltage scale for gas-filled detectors are Ionization Chambers, or Ion Chambers. They operate at a low voltage, meaning that the detector only registers a measurement from the “primary” ions (in actuality pair of ions created: a positively charged ion and a free electron) caused by an interaction with a radioactive photon in the reaction chamber.  Thus the measurement that the detector records is directly proportional to the number of ion pairs created. This is particularly useful as a measure of absorbed dose over time.  They are also valuable for the measurement of high-energy gamma rays, as they don’t have any of the issues with dead time that other detector types can have.

However, ion chambers are unable to discriminate between different types of radiation i.e. they cannot be used for spectroscopy. They can also tend towards being more expensive than other solution. Despite this, they are valuable detectors for survey meters. They are also widely used in laboratories to establish reference standards for calibrations.

PROPORTIONAL COUNTERS The next step up on the voltage scale for gas-filled detectors is the proportional (or gas-proportional) counter. They are generally devised so that for much of the area inside the chamber, they perform similarly to an ion chamber, in that interactions with radiation create ion pairs.  However , they have a strong enough voltage that the ions “drift” towards the detector anode.  As the ions approach the detector anode, the voltage increases, until they reach a point where a “gas amplification” effect occurs - the original ions created by the reaction with a photon of radiation causes further ionization reactions, which multiply the strength of the output pulse measured across the detector. The resulting pulse is proportional to the number of original ion pairs formed, which correlates to the energy of the radioactive field that it is interacting with .

The makes proportional counters very useful for some spectroscopy applications, since they react differently to different energies, and thus are able to tell the difference between different types of radiation that they come into contact with. They are also highly sensitive, which coupled with their effectiveness at alpha and beta detection and discrimination, makes this type of detector very valuable as a contamination screening detector.

GEIGER MULLER TUBE The Geiger-Mueller tube, the origin of the name “Geiger Counter.” Operating at a much higher voltage than other detector types, and differ from other detector types in that each ionization reaction, regardless of whether it is a single particle interaction or a stronger field, causes a gas-amplification effect across the entire length of the detector anode. Thus they can only really function as simple counting devices, used to measure count rates or, with the correct algorithms applied, dose rates . After each pulse, a G-M has to be “reset” to its original state.  This is accomplished by quenching. This can be accomplished electronically by temporarily lowering the anode voltage on the detector after each pulse, which allows the ions to recombine back to their inert state.

This can also be accomplished chemically with a quenching gas such as halogen which absorbs the additional photons created by an ionization avalanche without becoming ionized itself. Due to the extensive reaction G-M tubes experience with each pulse of radiation, they can experience something called “dead time” at higher exposure rates, meaning that there is a lag between the pulse cascade and when the gas is able to revert to its original state and be ready to detect another pulse. This can be accommodated for with calibration, or with algorithms in the detection instruments themselves to “calculate” what the additional pulses would be based on the existing measurement data.

Scintillators The 2 nd major type of detectors utilized in radiation detection instruments are Scintillation Detectors. Scintillation is the act of giving off light, and for radiation detection it is the ability of some material to scintillate when exposed to radiation that makes them useful as detectors. Each photon of radiation that interacts with the scintillator material will result in a distinct flash of light, meaning that in addition to being highly sensitive, scintillation detectors are able to capture specific spectroscopic profiles for the measured radioactive materials.

Scintillation detectors work through the connection of a scintillator material with a photomultiplier (PM) tube. The PM tube uses a photocathode material to convert each pulse of light into an electron, and then amplifies that signal significantly in order to generate a voltage pulse that can then be read and interpreted. The number of these pulses that are measured over time indicated the strength of the radioactive source being measured, whereas the information on the specific energy of the radiation, as indicated by the number of photons of light being captured in each pulse, gives information on the type of radioactive material present.

Due to their high sensitivity and their potential ability to “identify” radioactive sources, scintillation detectors are particularly useful for radiation security applications. These can take many forms, from handheld devices used to screen containers for hidden or shielded radioactive material, to monitors set up to screen large areas or populations, able to differentiate between natural or medical sources of radiation and sources of more immediate concern, such as Special Nuclear Material (SNM).

Solid State Detectors The last major detector technology used in radiation detection instruments are solid state detectors.  Generally using a semiconductor material such as silicon, they operate much like an ion chamber, simply at a much smaller scale, and at a much lower voltage. Semiconductors are materials that have a high resistance to electronic current, but not as high a resistance as an insulator. They are composed of a lattice of atoms that contain “charge carriers,” these being either electrons available to attach to another atom, or electron “holes,” or atoms with an empty place where an electron would/could be .

Silicon solid state detectors are composed of two layers of silicon semiconductor material, one “n-type,” which means it contains a greater number of electrons compared to holes, and one “p-type,” meaning it has a greater number of holes than electrons. Electrons from the n-type migrate across the junction between the two layers to fill the holes in the p-type, creating what’s called a depletion zone. This depletion zone acts like the detection area of an ion chamber.  Radiation interacting with the atoms inside the depletion zone causes them to re-ionize, and create an electronic pulse which can be measured.

The small scale of the detector and of the depletion zone itself means that the ion pairs can be collected quickly, meaning that the instruments utilizing this type of detector can have a particularly quick response time. This, when coupled with their small size, makes this type of solid state detector very useful for electronic dosimetry applications.  They are also able to withstand a much higher amount of radiation over their lifetime than other detectors types such as G-M Tubes, meaning that they are also useful for instruments operating in areas with particularly strong radiation fields.

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