CINCH NucWik

This page is read only. You can view the source, but not change it. Ask your administrator if you think this is wrong.
====== 10. Gas ionization detectors ======


Chapter 10 from BASICS OF NUCLEAR PHYSICS AND OF RADIATION DETECTION AND MEASUREMENT - An open-access textbook for nuclear and radiochemistry students by Jukka Lehto

  * [[#10.1._Ionization_chamber|Ionization chamber]]
  * [[#10.2._Proportional counter|Proportional counter]]
  * [[#10.3._Geiger-Műller counter|Geiger-Műller counter]]

###
Photons and particles emitted in [[textbook:nrctextbook:chapter5|radioactive decay]] [[textbook:nrctextbook:chapter7|ionize]] gas molecules which phenomenon is utilized in detection and [[textbook:nrctextbook:chapter8|measurement of radiation]]. In detectors based on the gas ionization, the ionizable gas is inside a metal chamber, which has typically a cylinder shape and is called tube. A voltage is applied to the tube so that the metal wall acts as cathode and a metal wire in the middle of the tube as anode ([[textbook:nrctextbook:chapter10#figure_101|Figure X.1]]).
###
{{anchor:figure_101}}
{{:textbook:nrctextbook:gas_ionization_detector_fig_10_1.png?200 |}}
Figure X.1. Gas ionization detector 
(http://www.equipcoservices.com/support/tutorials/introduction-to-radiation-monitors/).

{{anchor:gas_ionization_detector_function}}
###
[[textbook:nrctextbook:chapter5#5.4.1._gamma_decay|Gamma radiation]] penetrates the tube wall and ionizes the filling gas whereas [[textbook:nrctextbook:chapter5#5.3._beta_decay_processes|beta]] and [[textbook:nrctextbook:chapter5#5.2._alpha_decay|alpha]] radiations are not able to penetrate the wall. For the detection of alpha and beta active sources they either need to be placed inside the tube or the tube needs to have a penetrable window made of glass, mica or plastic. For the detection of external alpha radiation the window thickness should be very small. The filling gas is typically noble gas, such as argon, that the radiation ionizes to Ar<sup>+</sup> ions. Due to electric field applied between the electrodes these argon cations transfer towards the cathode, the tube wall, while the electrons transfer towards the anode, the metal wire in the middle of the tube. From the anode wire the electrons are transported through an external circuit to the tube wall where they neutralize Ar<sup>+</sup> ions back to Ar atoms. The electrons going through the external circuit are registered as an electric pulse representing an individual radiation absorption event. Thus, the number of electric pulses corresponds to the number of radiation absorptions in the tube which in turn corresponds to the number particles or photons hitting the tube, i.e. the number of pulses corresponds to the [[textbook:nrctextbook:chapter6#activity|activity]] of the source detected. As will be explained below the height of a pulse corresponds to the energy of a particle or a photon being absorbed in the tube in the case of two 
modes of gas ionization detectors ([[#10.1._Ionization_chamber|Ionization chamber]] and [[#10.2._Proportional counter|Proportional counter]]) but not in the third mode ([[#10.3._Geiger-Műller counter|Geiger-Műller counter]]). Depending on the voltage applied across the tube there are three types of gas ionization detectors ([[textbook:nrctextbook:chapter10#figure_102|Figure X.2]]).
###

{{anchor:figure_102}}

{{:textbook:nrctextbook:operation_ranges_of_gas_ionization_detectors_fig_10_2.png?200 |}} 

Figure X.2. Operation ranges of three gas ionization detectors as a function of high voltage applied across the tube (http://www.canberra.com/literature/fundamental-principles/).

{{anchor:ionization_chamber}}
{{anchor:recombination_area}}
===== 10.1. Ionization chamber =====

###
In the low voltage region, below about 50 V in Figure X.2, the velocities of the [[textbook:nrctextbook:chapter2#electron|electrons]] and the Ar<sup>+</sup> ion, induced by radiation absorption, towards the electrodes are so low that part of them are recombined back to Ar atoms before reaching the electrodes. This area (I in Figure X.2) is called recombination area. As the voltage is high enough to prevent recombination, all electrons and cations are collected to the electrodes. This area (II) is seen in Figure X.2 as about a 200 V wide area in the range of 130-330 V. In this range the number of ions (or electrons) collected on the electrodes is independent of the voltage applied. Gas ionization detectors operating at this voltage area are called //ionization chambers//. Since all ions and electrons are collected on the electrodes the height of the electric pulse recorded is proportional to the energy of the particle losing its kinetic energy in the filling gas. The higher is the initial energy the more there is [[textbook:nrctextbook:chapter7#ionization|ionization]] in the chamber and consequently the higher is the electric pulse recorded. [[textbook:nrctextbook:chapter5#alpha_particle|Alpha particles]] have typically very high energies and they also cause very high [[textbook:nrctextbook:chapter7#specific_ionization|specific ionization]]. Therefore, the pulses observed from alpha particles are much higher than those from [[textbook:nrctextbook:chapter5#beta_particle|beta particles]]. Ionization chambers are typically used for the detection of alpha radiation, for the measurement of absolute activities of radioactive sources and in radiation monitoring and dosimetry. In typical radionuclide laboratories, however, ionization chambers are very seldom used for activity measurements.
###
{{anchor:proportional_counter}}
===== 10.2. Proportional counter =====

###
As the voltage is further increased from ionization chamber operation range the electrons have such a high energy that they cause additional, [[textbook:nrctextbook:chapter7#secondary_ionization|secondary ionization]]. In this range (III) the height of the electric pulse is dependent on the voltage applied. A gas ionization detector working in this range is called //proportional counter// since the height of the electric pulse, at constant voltage, is proportional to the energy of the photon or particle losing its energy in the filling gas by ionizations. This is 
because the amplification of the electrons due to secondary ionizations is constant providing that the voltage remains the same. Thus, as in case of [[textbook:nrctextbook:chapter10#ionization_chamber|ionization chamber]] the proportional counter can be used in nuclear spectrometry, i.e. //in determination of alpha and beta particle energies//. As seen in Figure X.2 the amplification factor of electrons in proportional counters is up to about 10<sup>5</sup>. Since the pulse height is highly dependent on the voltage proportional counters need very stable high 
voltage sources. The advantage of proportional counter compared to ionization chamber is that the observed pulse is much higher and thus easier to detect.
###
{{anchor:gm_counter}}
===== 10.3. Geiger-Műller counter =====

###
As the voltage is further increased from the proportional counter area all individual particles or photons cause complete [[textbook:nrctextbook:chapter7#ionization|ionization]] of the filling gas (area IV). This means that the observed electric pulses have the same heigth and are thus independent of the energy of the particle or photon losing its energy in the tube. Thus //Geiger-Műller counter// cannot be used in nuclear spectrometry but only //in pulse counting//, i.e. determination of [[textbook:nrctextbook:chapter6#activity|activities]] or radiation intensities. The amplification of electrons in a Geiger-Műller tube is in the range 10<sup>6</sup>-10<sup>7</sup>. Thus, the pulses are in the volt range and no amplifiers are needed unlike in [[textbook:nrctextbook:chapter10#ionization_chamber|ionization chambers]] and [[textbook:nrctextbook:chapter10#proportional_counter|proportional counters]]. As seen in [[textbook:nrctextbook:chapter10#figure_102|Figure X.2]] the number of electrons (pulse height) is more or less constant in about 200 V wide voltage range. Since the plateau has not exactly a constant value the high voltage source needs to be stable. In good Geiger-Műller tubes the slope of the plateau is below 1%. As the voltage is still increased from the Geiger-Műller voltage range there will be a continuous electric discharge (area V) which can destroy the tube rather quickly.
###

###
In addition to argon (or neon) the filling gas in GM tubes contains about 10% of halogen or organic gas, such as ethyl alcohol, which act as quenching gases. As the argon ions approach the cathode or when they hit it, they may cause additional [[textbook:nrctextbook:chapter7#ionization|ionization]] which in turn causes additional erroneous pulses. As the ionization potentials of halogens and ethyl alcohol are lower than that of argon, Ar<sup>+</sup> ions transfer their positive charges to them when hitting them. These in turn do not cause additional ionization and their positive charge is neutralized on the surface of the cathode.

###
{{anchor:dead_time}} 
===== 10.4. Dead-time =====

###
When recording high pulse rates in [[#10.3._Geiger-Műller counter|GM tubes]] and in [[#10.2._Proportional counter|proportional counter]] (as also in most other radiation detectors) one needs to take into account the dead-time. As the argon gas ionizes, the induced electrons travel very fast to the anode while the positive argon ions travel much slower which causes a very low electric field near the anode (Figure X.3). The detector is then unable to record pulses that are caused from new radiation absorption events due to the travel of argon ions towards the cathode and recovery of the filling gas back to argon atoms. The time when the detector cannot record new pulses is called dead-time and it is marked with $\tau$.
###

{{:textbook:nrctextbook:pulse_shape_in_proportional_and_gm_counters_fig_10_3.png?400|}}

Figure X.3. Pulse shape in proportional and Geiger-Műller counters.

###
When so high count [[textbook:nrctextbook:chapter6|rates]] are measured that the dead-time becomes important the observed [[textbook:nrctextbook:chapter8#count_rate|count rates]] need to be corrected for dead-time $\tau$ (unit s). For that we mark observed count rate by $R$ (imp/s) and the true count rate by $R_0$ (imp/s) that would be observed if there was no dead-time. Because of the dead-time, $R_0 - R$ impulses in each second remain unrecorded. On the other in each second the tube is unable to record impulses a time $R \times \tau$ during which $R_0 \times R \times \tau$ photons or particles hit the detector. Thus
###


$$R_0 - R = R_0 \times R \times \tau$$;;#
[X.I]
;;#


from which we solve $R_0$

$$R_0 = \frac{R}{1 - R \times \tau}$$;;#
[X.II]
;;#

###
This equation can be used to correct the observed [[textbook:nrctextbook:chapter8#count_rate|count rate]] to true count rate as far as the dead-time of the tube is known. For example, if the observed count rate is 1000 imp/s and the dead-time is 0.2 ms the true count rate is $\frac{1000}{1 - 1000 \times 0.0002} = 1250 \, \text{imp/s}$ or 25% higher than the observed one. At ten times lower count rate 100 imp/s the true count rate is only 2% higher.
###


###
In [[textbook:nrctextbook:chapter10#gm_counter|GM tubes]] the dead-time is 0.1-0.4 ms while in [[textbook:nrctextbook:chapter10#proportional_counter|proportional counters]] it is much shorter, only a few microseconds. Therefore, a proportional counter can be used to measure a hundred times higher [[textbook:nrctextbook:chapter8#count_rate|count rates]] without the essential effect of dead-time. If proportional counter is used not only for pulse counting but also for nuclear spectrometry the highest count rates should, however, be avoided since the tube has, in addition to dead-time, also a recovery time (Figure X.3). If a new particle is recorded during the recovery time the pulse height response of the tube is higher than when each particle is recorded completely individually without overlap. The total recovery time in proportional counters is much higher than the dead-time, around 0.1 ms.
###

{{anchor:use_of_gm_and_proportional_counter}}
===== 10.5. Use of Geiger-Műller and proportional counters =====

###
Still in the 1950’s [[textbook:nrctextbook:chapter10#gm_counter|GM tubes]] were the most typical detectors for radiation measurements. For the activity measurements of individual [[textbook:nrctextbook:chapter4|radionuclides]], they needed to be first chemically separated from other radionuclides. Development of [[textbook:nrctextbook:chapter9#solid_scintillators|solid scintillation]] and [[textbook:nrctextbook:chapter9#semiconductor_detectors_gamma|semiconductor detectors]] have almost completely made chemical separation of gamma-emitting radionuclides unnecessary and thus also replaced gas ionization tubes in their measurements. Furthermore, [[textbook:nrctextbook:chapter12|liquid scintillation counting]] has mostly replaced measurement of beta-emitting radionuclides with gas ionization detectors. The gas ionization detectors are, however, still in extensive use, especially in radiation protection for the measurement or radiation doses and dose rates as well as in detection of surface contamination. In addition, GM tubes can be used in teaching since they are cheap and easy to operate and instead of more sophisticated equipment they can be used to demonstrate some basic features in radiation measurements. Basically, GM tubes can be used to measure all types of radiation. Gamma radiation is readily penetrating and [[textbook:nrctextbook:chapter8#counting_efficiency|counting efficiencies]] are only 1-2%. Thus GM tubes are used only for gamma dose and dose rate measurements. All beta and alpha particles entering the tube create electric pulse. However, to enter a tube the alpha and beta sources either need to be placed inside the tube or the window between the source and the tube should be very thin. For alpha radiation the thin window is made of plastics and these types of tubes are used to detect alpha contamination from various surfaces. For beta radiation the thin (0.1 mm) windows are made of mica, glass or beryllium but even these are too thick to allow measurement of the lowest beta energies, such 18 keV beta energies of tritium. Even though scintillation counting today is a standard method for beta counting, a gas ionization detector has one important advantage over it: the background is much lower which enables measurement of lower activities. An example of such equipment is the Risö 
Beta Counter (Figure X.4) which is a rather simple equipment and easy to operate. It has five sample positions for sources prepared after chemical separation and individual GM-tubes for each sample position. The samples are shielded against external radiation by lead shield and a guard counter that detects external radiation passing through the lead shield and subtracts the count rate observed in the guard detector from the total observed count rate. With this equipment the background count rate is typically only 0.2 cpm compared to at least ten times higher background 
observed with liquid scintillation counting.
###

{{:textbook:nrctextbook:riso_beta_counter_fig_10_4.png?400|}}

Figure X.4. Risö Beta Counter (http://www.nutech.dtu.dk/english/Products-and-Services/Dosimetry/Radiation-Measurement-Instruments/GM_multicounter).

###
//Neutrons as neutral particles do not cause any ionization in gas ionization detectors//. To detect neutrons the tube is filled with BF<sub>3</sub> gas where boron is enriched with respect to <sup>10</sup>B [[textbook:nrctextbook:chapter2#isotope|isotope]]. In this gas the neutrons cause the following nuclear reaction:
###

$$^{10}\text{B} + n \rightarrow {}^7\text{Li} + {}^4\text{He}$$ ;;#
[X.III]
;;#

###
and the emitted [[textbook:nrctextbook:chapter5#5.2._alpha_decay|alpha particles]] and the recoiled lithium atoms cause [[textbook:nrctextbook:chapter7#ionization|ionization]] of the gas which makes the neutron detection and counting possible.
###
CINCH NucWik

Sidebar

A-CINCH Consortium

CINCH NucWik

User Tools

Site Tools

Sidebar

Page Tools

A-CINCH Consortium
