|
|||||||||||||||||||
|
See also ... |
|||||||||||||||||||
|
|||||||||||||||||||
|
In the previous section, we discussed the deleterious effects that radiation can have on human beings (and indeed animals). This rather gives the impression that one should strive at all costs to avoid any sort of exposure to radiation! However, this is quite impossible, as radiation is all around us, and we are continually bombarded with radioactive particles.
The level of radiation exposure from natural sources occurs
at the level of stochastic effects, discussed in the previous section, and the
principal sources are as follows:
1.
Cosmic rays;
2.
Naturally occurring radionuclides in soils and rock;
3.
Naturally occurring radionuclides in our bodies;
4.
Radon gas in our homes
We will
discuss each of these in turn.
Cosmic Rays
Cosmic
rays are a source of radiation that originates from outer space.
In fact there are two sources; the first is the sun, with the remainder
originating from outside the solar system.
Primary cosmic rays (those that are incident on the atmosphere of the
earth) consist mainly of protons (hydrogen nuclei), and alpha particles (helium
nuclei). Also present are electrons
and a small number of heavier nuclei.
The
energy of the primary cosmic rays can be very high, and when these cosmic rays
interact with the atoms and molecules in the atmosphere, a number of additional
secondary particles are produced, including protons, electrons, neutrons,
positrons and a variety of more ‘exotic’ particles that will not be
discussed here. Many of these
secondary cosmic rays are sufficiently energetic to reach the surface of the
earth.
At sea
level, it has been found that the number of ions produced by cosmic rays is
about 2 ions per cubic centimeter per second.
Using this information, it can be calculated that the absorbed dose rate
due to these cosmic rays is about 32 nGy/hr (0.000000032 Gy/hr).
The world average annual dose rate due to cosmic rays is about 0.4 mSv/yr
(0.0004 Sv/yr).
It is of
interest to note that the dose rate due to cosmic rays increases with altitude,
because the flux of cosmic ray particles increases (they have less distance to
travel through the earth’s atmosphere). Thus,
regular travellers by airplane, and indeed the pilots of those planes, will be
subject to considerably higher radiation doses.
The dose rate doubles for every 1500 m increase in altitude, and so at a
cruising height of 10000 m, the dose rate could exceed 32 nGy/hr
´
2(10/1.5) ~ 3.2
mGy/hr.
This is 100 times greater than the dose rate at sea level.
Supersonic
aircraft often fly at much higher altitudes, perhaps as high as 15 km.
The dose rate at this altitude could be as high as 210
´
32 nGy/hr = 33
mGy/hr.
It is reassuring to note that supersonic aircraft carry monitoring
equipment to measure the cosmic ray dose rate, so that during periods of intense
cosmic radiation (for example during solar flares – the primary source of
solar cosmic radiation), the pilot can adopt a lower flying height, resulting in
a reduction of the radiation dose to the passengers and crew.
Radionuclides in Soils and Rock
A number
of radioactive materials occur naturally in the earth itself.
These radioactive materials all have very long half lives, and have been
present in the earth since its creation. At
the creation of the earth during the Big Bang, perhaps about 15 billion years
ago, virtually all possible atoms were created.
Most of the radioactive atoms will have decayed away, but there are three
important radionuclides that have such long half lives that even after 15
billion years, they are still present in the earth.
These radionuclides are:
Uranium-238
half life = 4.46 billion years;
Thorium-232
half life = 14 billion years
Potassium-40
half life = 1.3 billion years
Other
primordial radionuclides include rubidium-87 and uranium-235, but these are not
so important in considering radiation doses to man. Uranium-235 is an important source of fuel for many types of
nuclear reactor, and the extraction of concentrated amounts of uranium-235 from
natural uranium in the ground is a major technological challenge.
Uranium-238
and thorium-232 have the important property that their radioactive decay
products are also radioactive. Both
of these nuclides are at the beginning of long sequences of radionuclides
(containing about 10 or 15 members) in which each member is radioactive, and
decays to the next member in the series. Only
the final member of the series consists of stable atoms.
Uranium-235 is also at the head of a long sequence of radionuclides.
The
following diagram illustrates these two radionuclides and the radioactive
progeny that arise from their decay.
It
follows that any of the members of the decay series mentioned above can give
rise to a radiation dose to man. However,
the nature of the radiation dose is usually considered in two categories, namely
external doses, and doses that arise internally, for example because the
nuclides have been inhaled or ingested. It
turns out that the external doses from these natural nuclides are dominated by
bismuth-214, which is a strong gamma emitter and occurs in the uranium-238
series, and thallium-208, which is also a gamma emitter and occurs in the
thorium-232 series. The external
dose, averaged over the world population, is about 0.5 mSv/yr. The internal doses arise when radioactive materials are ingested or inhaled. In this case, the nuclides that emit alpha particles assume a greater importance (for example radium-226 in the uranium-238 series). The dose arising from internal contamination (averaged over the world population) is about 0.3 mSv/yr.
Radionuclides in the Body
An
important radionuclide that can be found in the human body is potassium-40 (it
is also found in soils and rocks, and contributes to the doses considered in the
previous section). The human body
of a 70 kg man contains about 140 g of potassium, most of which is located in
muscle. Of this potassium, about
0.018% is radioactive potassium-40. This
corresponds to a mass of potassium-40 of about 0.03 g.
It can be shown by calculation that the decay of this potassium-40
produces about 6000 radioactive decays every second, and therefore body tissues
will acquire a radiation dose. The
dose arising from potassium-40 in the body (and a contribution due to naturally
occurring potassium-40 in rocks and soils) is about 0.1 mSv/yr.
Radon in Homes
One of
the most important sources of natural radiation arises from an element called
radon. The two most important
isotopes of radon are radon-220 and radon-222.
The former is often called thoron
and the latter is usually given the name of the element, i.e. radon.
To avoid confusion, we will reserve the term radon
for the name of the element, and we will refer to each isotope explicitly.
Radon
has two important qualities from the perspective of radiation protection:
1.
Radon is a gas;
2.
Both isotopes of radon are radioactive and are derived either from the
decay of uranium-238 (radon-222) or thorium-232 (radon-220).
Thus,
because uranium-238 and thorium-232 occur to some extent in all soils and rocks,
it follows that radon gas is constantly emanating from the ground.
In areas that are particularly rich in uranium and/or thorium ores, the
rate of emanation can be quite high. However,
the radiological hazard from radon-220 (thoron) is usually smaller than that
from radon-222, because radon-220 has a half-life of only 55 seconds, and so
decays away before radiological problems can arise.
Radon is colourless and odourless, so we cannot perceive the presence of
radon in the atmosphere. However,
in most circumstances, only radon-222 is problematic.
Of
particular importance is the fact radon can accumulate in enclosed structures
such as homes and offices. The
radon either seeps into buildings through the foundations, or in parts of the
world where building materials are derived from local sources, the radon may
enter the building as a result of emanation from the foundation and building
materials themselves. If the degree
of ventilation of the building is negligible, radon can accumulate to
substantial levels. The
radiological hazard is exacerbated by the fact that buildings such as homes tend
to be occupied for substantial periods of time.
Strictly
speaking, radon-222 itself is not particularly dangerous, as radon is an inert
gas, and so radon breathed in tends to be breathed straight back out again.
However, the decay products of radon-222 are isotopes of bismuth and
polonium, which are ‘heavy’ metals that attach themselves to dust particles,
and tend to accumulate in the lung. These
isotopes then undergo further radioactive decay, and bombard the lungs with
alpha particles, resulting in radiological damage to the cells of the lung.
Thus, lung cancer is a possible outcome from exposure to radon.
It should be noted that cigarette smoking tends to increase the
likelihood of lung cancer in regions where radon levels are high.
The
hazard of radon is taken so seriously that action
levels are defined in most countries. These
action levels specify the maximum concentration of radon and its decay products
that is allowed before intervention is required to lower concentrations.
The most common type of intervention is the use of fans under the floor
of an affected building to ‘suck’ radon out of the underfloor region, before
it can enter the main volume of the building.
Ionising Radiation - The End
At this
point, it was my intention to describe some of the more practical uses of
radiation. However, it became clear
to me that (1) there are so many uses that I could not do justice to them all;
(2) I may never actually finish writing this article if I started out to do
that, and; (3) people’s views differ on what are acceptable, unacceptable or
controversial uses. There are a multitude of stories (both happy and sad) about how people’s lives have been changed as a result of radiation. But that’s for another time!
Index | Site Map | Photos | Videos | Science | England | London | Cars | Dogs | Albania | Diary 9-11| Author | Links | Contact |
|||||||||||||||||||