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Atomic absorption spectrometry

原子吸收光谱(AAS)

  • Atomic absorption spectrometry (AAS) is an
    analytical technique that measures the
    concentrations of elements. Atomic absorption is so
    sensitive that it can measure down to parts per billion
    of a gram (μg dm–3) in a sample. The technique
    makes use of the wavelengths of light specifically
    absorbed by an element. They correspond to the
    energies needed to promote electrons from one
    energy level to another, higher, energy level.
    Atomic absorption spectrometry has many uses in
    different areas of chemistry.
    Clinical analysis. Analysing metals in biological
    fluids such as blood and urine.
    Environmental analysis. Monitoring our
    environment – eg finding out the levels of various
    elements in rivers, seawater, drinking water, air,
    petrol and drinks such as wine, beer and fruit drinks.
    Pharmaceuticals. In some pharmaceutical
    manufacturing processes, minute quantities of a
    catalyst used in the process (usually a metal) are
    sometimes present in the final product. By using
    AAS the amount of catalyst present can be
    determined.
    Industry. Many raw materials are examined and
    AAS is widely used to check that the major elements
    are present and that toxic impurities are lower than
    specified – eg in concrete, where calcium is a major
    constituent, the lead level should be low because it is
    toxic.
    Mining. By using AAS the amount of metals such as
    gold in rocks can be determined to see whether it is
    worth mining the rocks to extract the gold.
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  • 第1楼2005/04/02

    How it works
    Atoms of different elements absorb characteristic
    wavelengths of light. Analysing a sample to see if it
    contains a particular element means using light from
    that element. For example with lead, a lamp
    containing lead emits light from excited lead atoms
    that produce the right mix of wavelengths to be
    absorbed by any lead atoms from the sample. In
    AAS, the sample is atomised – ie converted into
    ground state free atoms in the vapour state – and a
    beam of electromagnetic radiation emitted from
    excited lead atoms is passed through the vaporised
    sample. Some of the radiation is absorbed by the lead
    atoms in the sample. The greater the number ofatoms there is in the vapour, the more radiation is
    absorbed. The amount of light absorbed is
    proportional to the number of lead atoms. A
    calibration curve is constructed by running several
    samples of known lead concentration under the same
    conditions as the unknown. The amount the
    standard absorbs is compared with the calibration
    curve and this enables the calculation of the lead
    concentration in the unknown sample.
    Consequently an atomic absorption spectrometer
    needs the following three components: a light source;
    a sample cell to produce gaseous atoms; and a means
    of measuring the specific light absorbed.

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  • 第2楼2005/04/02

    The light source
    The common source of light is a ‘hollow cathode
    lamp’ (Fig. 1). This contains a tungsten anode and a
    cylindrical hollow cathode made of the element to be
    determined. These are sealed in a glass tube filled
    with an inert gas – eg neon or argon – at a pressure o

    between 1 Nm–2 and 5 Nm–2. The ionisation of some
    gas atoms occurs by applying a potential difference of
    about 300–400 V between the anode and the
    cathode. These gaseous ions bombard the cathode
    and eject metal atoms from the cathode in a process
    called sputtering. Some sputtered atoms are in
    excited states and emit radiation characteristic of the
    metal as they fall back to the ground state – eg
    Pb* → Pb + h (Fig. 2). The shape of the cathode
    concentrates the radiation into a beam which passes
    through a quartz window, and the shape of the lamp
    is such that most of the sputtered atoms are
    redeposited on the cathode.

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  • 第3楼2005/04/02


    A typical atomic absorption instrument holds
    several lamps each for a different element. The lamps
    are housed in a rotating turret so that the correct
    lamp can be quickly selected.

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  • 第4楼2005/04/02

    The optical system and detector
    A monochromator is used to select the specific
    wavelength of light – ie spectral line – which is
    absorbed by the sample, and to exclude other
    wavelengths. The selection of the specific light allows
    the determination of the selected element in the
    presence of others. The light selected by the
    monochromator is directed onto a detector that is
    typically a photomultiplier tube. This produces an
    electrical signal proportional to the light intensity
    (Fig. 3).
    Double beam spectrometers
    Modern spectrometers incorporate a beam splitter so
    that one part of the beam passes through the sample
    cell and the other is the reference (Fig. 4). The
    intensity of the light source may not stay constant
    during an analysis. If only a single beam is used to pass
    through the atom cell, a blank reading containing no
    analyte (substance to be analysed) would have to be
    taken first, setting the absorbance at zero. If the
    intensity of the source changes by the time the
    sample is put in place, the measurement will be
    inaccurate. In the double beam instrument there is a
    constant monitoring between the reference beam and
    the light source. To ensure that the spectrum does not
    suffer from loss of sensitivity, the beam splitter is
    designed so that as high a proportion as possible of
    the energy of the lamp beam passes through the
    sample.

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  • 第6楼2005/04/02

    Atomisation of the sample
    Two systems are commonly used to produce atoms
    from the sample. Aspiration involves sucking a
    solution of the sample into a flame; and
    electrothermal atomisation is where a drop of sample
    is placed into a graphite tube that is then heated
    electrically.
    Some instruments have both atomisation systems
    but share one set of lamps. Once the appropriate lamp
    has been selected, it is pointed towards one or other
    atomisation system.

    Flame aspiration
    Figure 5 shows a typical burner and spray chamber.
    Ethyne/air (giving a flame with a temperature of
    2200–2400 °C) or ethyne/dinitrogen oxide (2600–
    2800 °C) are often used. A flexible capillary tube
    connects the solution to the nebuliser. At the tip of
    the capillary, the solution is ‘nebulised’ – ie broken
    into small drops. The larger drops fall out and drain
    off while smaller ones vaporise in the flame. Only
    ca 1% of the sample is nebulised.

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  • 第8楼2005/04/02

    Electrothermal atomisation
    Figure 6 shows a hollow graphite tube with a platform.
    25 μl of sample (ca 1/100th of a raindrop) is placed
    through the sample hole and onto the platform from
    an automated micropipette and sample changer. The
    tube is heated electrically by passing a current
    through it in a pre-programmed series of steps. The
    details will vary with the sample but typically they
    might be 30–40 seconds at 150 °C to evaporate the
    solvent, 30 seconds at 600 °C to drive off any volatile
    organic material and char the sample to ash, and with
    a very fast heating rate (ca 1500 °C s-1) to 2000–
    2500 °C for 5–10 seconds to vaporise and atomise
    elements (including the element being analysed).
    Finally heating the tube to a still higher temperature
    – ca 2700 °C – cleans it ready for the next sample.
    During this heating cycle the graphite tube is flushed
    with argon gas to prevent the tube burning away. In
    electrothermal atomisation almost 100% of the
    sample is atomised. This makes the technique much
    more sensitive than flame AAS.

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  • 第9楼2005/04/02

    Sample preparation
    Sample preparation is often simple, and the chemical
    form of the element is usually unimportant. This is
    because atomisation converts the sample into free
    atoms irrespective of its initial state. The sample is
    weighed and made into a solution by suitable
    dilution. Elements in biological fluids such as urine
    and blood are often measured simply after a dilution
    of the original sample. Figure 7 shows a flame atomic
    absorption spectrometer with an autosampler and
    flow injection accessory.
    When making reference solutions of the element
    under analysis, for calibration, the chemical
    environment of the sample should be matched as
    closely as possible – ie the analyte should be in the
    same compound and the same solvent. Teflon
    containers may be used when analysing very dilute
    solutions because elements such as lead are sometimes
    leached out of glass vessels and can affect the results.

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  • 第10楼2005/04/02

    Background absorption
    It is possible that other atoms or molecules apart from
    those of the element being determined will absorb or
    scatter some radiation from the light source. These
    species could include unvaporised solvent droplets, or
    compounds of the matrix (chemical species, such as
    anions, that tend to accompany the metals being
    analysed) that are not removed completely. This
    means that there is a background absorption as well as
    that of the sample.
    One way of measuring and correcting this
    background absorption is to use two light sources, one
    of which is the hollow cathode lamp appropriate to
    the element being measured. The second light source
    is a deuterium lamp.
    The deuterium lamp produces broad band
    radiation, not specific spectral lines as with a hollow
    cathode lamp. By alternating the measurements of the
    two light sources – generally at 50 –100 Hz – the
    total absorption (absorption due to analyte atoms plus
    background) is measured with the specific light from
    the hollow cathode lamp and the background
    absorption is measured with the light from the
    deuterium lamp. Subtracting the background from the
    total absorption gives the absorption arising from only
    analyte atoms.

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