Name: atomic emission spectroscopy for element analysis
Uploaded: 2024-12-05T18:32:15.000Z
Duration: 1 min 20 s
Channel: JoVE

K12 Standards

Pennsylvania State Academic Standards

9-12

Earth and Space Science

Space Systems

3.3.9-12.C

Atomic Emission Spectroscopy: Overview

Atomowa spektroskopia emisyjna (AES) umożliwia analizę wieloelementową próbki, w której wszystkie anality mogą być jednocześnie wzbudzane przez wyładowanie elektryczne, płomień lub plazmę.
W AES atomy w stanie wzbudzonym rozluźniają się, dając charakterystyczne emisje, a intensywność emisji jest wprost proporcjonalna do populacji w stanie wzbudzonym.
Znaczne populacje atomów w stanie wzbudzonym uzyskuje się dzięki zastosowaniu wysokotemperaturowej plazmy argonowej.
Plazma argonowa – gorąca, elektrycznie przewodząca gazowa mieszanina jonów argonu i elektronów – jest generowana przez jonizację przepływającego strumienia argonu. Plazma jest podtrzymywana w nieskończoność przez zasilacz, który utrzymuje optymalną temperaturę do dalszej jonizacji. 
Źródło plazmy o częstotliwości radiowej, zwane plazmą sprzężoną indukcyjnie lub ICP, może osiągać temperatury do 10 000 K. Jest to szeroko stosowane źródło wzbudzenia w AES, powszechnie określane jako ICP-AES lub ICP-OES.
Inne źródła plazmy obejmują plazmę indukowaną mikrofalami, plazmę prądu stałego, mikroplazmę i plazmę indukowaną laserem.

spektroskopia emisyjna atomów: przegląd

Spektroskopia emisyjna atomów (AES) to technika analityczna stosowana do określania składu pierwiastkowego próbki poprzez analizę światła emitowanego przez wzbudzone atomy. W AES atomy w próbce są wzbudzane do wyższych poziomów energii przez energię cieplną ze źródeł wysokotemperaturowych, takich jak plazma, łuki lub iskry. Kiedy te wzbudzone atomy powracają do niższych stanów energetycznych, emitują światło o określonych długościach fal charakterystycznych dla każdego pierwiastka. Powstałe widmo emisji atomów, które składa się z dyskretnych linii odpowiadających tym długościom fal, umożliwia identyfikację i kwantyfikowanie różnych pierwiastków w próbce.

 Instrumentacja AES ma podobieństwa do spektrometrów absorpcji atomowej, ale ze specyficznymi adaptacjami do wykrywania emisji. Źródła wysokotemperaturowe, w szczególności plazma sprzężona indukcyjnie (ICP), są niezbędne w AES, ponieważ osiągają wystarczającą energię, aby wzbudzić atomy do ich stanów emisji. Inne źródła plazmy obejmują plazmę indukowaną mikrofalami (MIP) i plazmę prądu stałego (DCP). Najczęściej stosowane źródło, ICP, osiąga temperatury do 10 000 K, tworząc stabilne środowisko dla spójnego wzbudzenia i emisji. ICP-AES, znane również jako ICP-OES (spektrometria emisji optycznej), umożliwia analizę wieloelementową poprzez umieszczenie wielu detektorów w półkolistym układzie wokół źródła emisji w celu uchwycenia jednoczesnych odczytów w zakresie długości fal.

 AES oferuje kilka zalet w porównaniu z tradycyjnymi metodami absorpcji atomowej, takimi jak techniki płomieniowe i elektrotermiczne. Ze względu na źródła wysokotemperaturowe, które dysocjują złożone cząsteczki, AES jest mniej podatny na zakłócenia chemiczne, umożliwiając czystsze odczyty widmowe. Technika ta umożliwia jednoczesną analizę wieloelementową, znacznie poprawiając wydajność analityczną. Ponadto AES obejmuje szerszy zakres stężeń, dzięki czemu nadaje się do różnych typów próbek.

 Pomimo tych zalet AES ma ograniczenia. Złożone widma wytwarzane przez źródła wysokotemperaturowe zwiększają prawdopodobieństwo zakłóceń widmowych, co komplikuje analizę ilościową. Aby sprostać tym wyzwaniom, instrumenty AES wymagają systemów optycznych o wysokiej rozdzielczości, często droższych niż te stosowane w spektrometrii absorpcji atomowej. Ponadto, podczas gdy AES jest skuteczną metodą do analizy wielu pierwiastków, techniki absorpcji atomowej pozostają cenne w analizie pojedynczych pierwiastków ze względu na ich prostotę, opłacalność i precyzję.

 AES jest szeroko stosowany w monitorowaniu środowiska, materiałoznawstwie i laboratoriach klinicznych do analizy metali, pierwiastków śladowych i innych substancji nieorganicznych. Jego zdolność do wykonywania szybkiej analizy wielopierwiastkowej sprawia, że ​​AES jest szczególnie przydatny do testowania próbek gleby, wody i próbek biologicznych. Wysoka czułość i szeroki zakres pierwiastków instrumentów AES umożliwiają dokładne pomiary zarówno w stężeniach śladowych, jak i znaczących, co czyni go wszechstronnym narzędziem do analizy pierwiastkowej w różnych dziedzinach nauki.

 W AES analiza ilościowa polega na pomiarze intensywności emitowanego światła, które jest proporcjonalne do populacji wzbudzonych atomów. Zgodnie z rozkładem Boltzmanna ta populacja stanów wzbudzonych zależy od temperatury źródła wzbudzenia, przy czym wyższe temperatury powodują większe emisje. Krzywe kalibracji, często liniowe w zakresie kilku rzędów wielkości, są tworzone poprzez analizę znanych standardów w celu skorelowania intensywności emisji ze stężeniami pierwiastków. Techniki standaryzacji są kluczowe dla kontrolowania zmian w wydajności wzbudzenia i innych czynników instrumentalnych, umożliwiając dokładną kwantyfikację pierwiastków w różnych próbkach.

Spektroskopia emisyjna atomów: przegląd

Atomowa spektroskopia emisyjna (AES) to technika analityczna stosowana do określania składu pierwiastkowego próbki poprzez analizę światła emitowanego z ...

Education

JoVE Core

Analytical Chemistry

Chemia analityczna

Unit 1

Jednostka 1

Atomic Spectroscopy

Spektroskopia atomowa

KEY TERMS AND CONCEPTS

KLUCZOWE TERMINY I POJĘCIA

atomic emission spectroscopy for element analysis

Atomic emission spectroscopy is used to identify the elements in a sample by measuring the light they emit. Atoms are first excited to higher energy levels by thermal energy from hot sources such as plasma, arcs, or sparks. When they fall back to lower energy levels, they give off light at specific wavelengths. Each element produces its own set of lines, so the emission spectrum can show both what is present and how much is there.

AES instruments are similar to atomic absorption spectrometers, but they are built to detect emitted light. High-temperature sources are essential because they provide enough energy to excite atoms into their emission states. Inductively coupled plasma, or ICP, is the most widely used source. It can reach temperatures up to 10,000 K and creates a stable environment for steady excitation and emission. Other plasma sources used in AES include microwave-induced plasma, or MIP, and direct current plasma, or DCP.

ICP-AES is also called ICP-OES, which stands for optical emission spectrometry. This setup allows multielement analysis by placing multiple detectors in a semicircular array around the emission source. The detectors can record several wavelengths at the same time. That makes the method fast and useful when more than one element must be measured in the same sample.

AES has several advantages over traditional atomic absorption methods such as flame and electrothermal techniques. The high-temperature source helps break apart complex molecules, so chemical interferences are usually lower. The method also supports simultaneous multielement analysis, which improves efficiency. In addition, AES covers a wider concentration range, so it works with many different sample types.

The technique also has limits. High-temperature sources create complex spectra, which increases the chance of spectral interferences and can make quantitative analysis harder. AES instruments need high-resolution optical systems to separate the lines clearly, and these systems are often more expensive than those used in atomic absorption spectrometry. For single-element analysis, atomic absorption methods are still useful because they are simple, cost-effective, and precise.

AES is widely used in environmental monitoring, materials science, and clinical laboratories. It can analyze metals, trace elements, and other inorganic substances in soil, water, and biological samples. This makes it valuable for rapid testing across many scientific fields. The method is sensitive and can measure both trace and significant concentrations.

Quantitative AES depends on the intensity of the emitted light. That intensity is related to the number of atoms in the excited state. According to the Boltzmann distribution, this excited-state population depends on the temperature of the source, so higher temperatures produce more emission. To find concentration, scientists use calibration curves made from known standards, and they apply standardization methods to reduce the effects of changes in excitation efficiency and other instrument factors.

Atomic Emission Spectroscopy for Element Analysis

atomic-emission-spectroscopy-for-element-analysis

atomic spectroscopy: absorption, emission, and fluorescence

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Element Analysis with Atomic Light Spectra

Atomic spectroscopy is used to identify and measure elements by their light signals. It supports both qualitative analysis, which tells what is present, and quantitative analysis, which tells how much is present. The optical methods in this group are atomic absorption spectroscopy, atomic emission spectroscopy, and atomic fluorescence spectroscopy. These methods begin with atomization. In this step, a solid, liquid, or solution sample is changed into gas-phase atoms and ions. Once the sample...

atomic spectroscopy: effects of temperature

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How Heat Changes Atomic Spectra

Heat changes atomic spectra by affecting atomization, excitation, ionization, and line shape. In atomic spectroscopy, atomization means converting a sample into gas-phase atoms and ions. The flame temperature needed for this step changes how efficiently the method works and shifts the balance between excited and ground-state atoms. At thermal equilibrium, the relative numbers of excited and ground-state atoms can be estimated with the Maxwell-Boltzmann distribution. A small temperature rise...

atomic absorption spectroscopy: overview

Atomic Absorption Spectroscopy for Trace Metals

Atomic absorption spectroscopy (AAS) measures trace metals by tracking how atoms absorb electromagnetic radiation (EMR). The absorbed light makes atoms move to a higher-energy orbit. In AAS, the key step is atomization, which converts the sample into gas-phase atoms. A flame or a furnace is typically used for this step. Inside the flame, some atoms become thermally excited. Most stay in the ground state, which is the lowest-energy state. These ground-state gas-phase atoms absorb EMR only when...

atomic absorption spectroscopy: instrumentation

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Atomic Absorption Spectroscopy: Key Parts

Atomic absorption spectrophotometry uses a set of key parts to measure light absorbed by atoms. The main components are a radiation source, an atomizer, a monochromator, and a detector. Each part has a specific job in the instrument. The radiation source is usually a hollow-cathode lamp, or HCL, or an electrodeless-discharge lamp, or EDL. Both produce a narrow emission line at the needed wavelength. Some instruments instead use continuum sources with high-resolution monochromators to narrow...

atomic absorption spectroscopy: radiation and light sources

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Choosing Light Sources for AAS Measurements

Atomic absorption spectroscopy (AAS) uses a light source that emits a very narrow range of wavelengths. This is needed because the source must match the absorption behavior of the analyte atom. The choice of source also depends on giving a precise, intense emission at the right wavelength for accurate detection. Two common line sources in AAS are hollow-cathode lamps (HCLs) and electrodeless-discharge lamps (EDLs). These lamps are selected based on the element being analyzed and the level of...

atomic absorption spectroscopy: atomization methods

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Atomic Absorption Spectroscopy: Sample Atomization

Atomic absorption spectroscopy uses sample atomization to turn a liquid specimen into free atoms for analysis. The two main approaches are flame atomization and electrothermal atomization. Both methods prepare the sample so its atoms can be measured by the instrument. Flame atomization uses a nebulizer and spray chamber to mix the sample with a fuel-oxidant mixture. This creates a fine aerosol mist that enters the burner. The fuel and oxidant are usually close to a stoichiometric ratio, but a...

atomic absorption spectroscopy: interference

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Correcting Errors in Atomic Absorption Spectroscopy

Atomic absorption spectroscopy interference can create systematic error by making the analytical signal or the background look stronger or weaker than it should be. In atomic absorption measurements, these errors are usually grouped as spectral interference, chemical interference, and physical interference. Spectral interference happens when signals from other elements or molecules overlap with the analyte signal, the substance being measured. This overlap can falsely raise or hide the analyte...

atomic absorption spectroscopy: lab

AAS Sample Prep and Calibration

Atomic absorption spectroscopy (AAS) depends on careful sample preparation and calibration. Samples must be turned into clear solutions before measurement. That often means extra treatment to dissolve materials such as soils, animal tissues, and minerals. Common sample prep methods include hot mineral acids, wet ashing, combustion in closed containers, high-temperature ashing, and fusion with reagents. These steps help make the sample suitable for AAS analysis. Solutions that contain organic...

atomic emission spectroscopy: overview

Atomic emission spectroscopy is used to identify the elements in a sample by measuring the light they emit. Atoms are first excited to higher energy levels by thermal energy from hot sources such as plasma, arcs, or sparks. When they fall back to lower energy levels, they give off light at specific wavelengths. Each element produces its own set of lines, so the emission spectrum can show both what is present and how much is there. AES instruments are similar to atomic absorption spectrometers,...

atomic emission spectroscopy: instrumentation

atomic-emission-spectroscopy-instrumentation

AES Sample Handling and Detection

Atomic emission spectrometry (AES) uses sample handling, atomization, and detection parts to measure emitted light from atoms and ions. The sample must first be changed into a gas-phase form so it can produce a measurable signal. AES uses two main atomizer types. Continuous atomizers, such as flames and plasmas, feed the sample in a steady stream. Discrete atomizers add one sample at a time with syringes or autosamplers. The electrothermal atomizer is the most common discrete type. Many...

atomic emission spectroscopy: interference

atomic-emission-spectroscopy-interference

Reducing Interference in AES Signals

Atomic emission spectroscopy (AES) can produce interfering signals when atoms and molecules in a flame or plasma emit overlapping light. High-temperature atomizers excite many species at once, including oxides, hydroxides, and flame combustion products. These extra emissions can make the analyte signal harder to read. Spectral interference happens when emission lines or bands overlap. One way to reduce it is to improve instrument resolution. Another is to choose a different emission line for...

inductively coupled plasma atomic emission spectroscopy: principle

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ICP-AES Torch and Sample Analysis

Inductively coupled plasma atomic emission spectroscopy uses a plasma torch to analyze elements in a sample. This method is also called inductively coupled plasma optical emission spectroscopy, or ICP-OES. It is widely used because the plasma creates a strong environment for elemental analysis. The ICP source, or torch, contains three concentric quartz tubes. Argon gas flows through the tubes. A spark from a Tesla coil starts the ionization of argon and creates a high-temperature plasma. The...

inductively coupled plasma atomic emission spectroscopy: instrumentation

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ICP-AES Instrument Types and Detection

Inductively coupled plasma atomic emission spectroscopy, or ICP-AES, uses an inductively coupled plasma to detect and analyze elements in a sample. The method measures the light given off by atoms, which helps identify and compare different elements. It is a common approach in atomic emission spectroscopy. ICP-AES instruments are built in three main forms: sequential, simultaneous multichannel, and Fourier transform instruments. Fourier transform designs are less commonly used, but they are...

atomic emission spectroscopy: lab

Plasma Sources in Atomic Emission Spectroscopy

Atomic emission spectroscopy uses plasma sources to identify elements by their light. The method creates abundant spectra with characteristic emission lines. Inductively coupled plasma, or ICP, is especially useful because it gives strong quantitative data. It works well under stable conditions, with low noise, low background, and few interferences. Newer air-operated microwave sources are also being studied. These sources may be more cost-effective than conventional ICP systems. Atomic...

atomic fluorescence spectroscopy

Measuring Elements by Atomic Fluorescence

Atomic fluorescence spectroscopy measures elements by detecting the light atoms give off after they are excited by electromagnetic radiation. The atoms are first placed in a flame, furnace, or plasma. They absorb energy, become excited, and then release that energy as they return to their original state. The emitted light is called fluorescence. The fluorescence is observed at a right angle to the incoming beam. This setup helps separate the emitted light from the light used to excite the...

flame photometry: overview

Flame Emission Spectrometry Basics

Flame emission spectrometry uses a flame to excite elements in a sample so their light can be measured. It is also called flame photometry. The method can be used for both qualitative and quantitative analysis of elements. The idea became established in the early 1860s when Kirchhoff and Bunsen showed that specific elements give off characteristic radiation in a flame. The first instrument for this purpose measured sodium in plant ash with a Bunsen flame. A major problem was how to add the...

flame photometry: lab

Flame Photometry and Metal Detection

Flame photometry is a method for detecting metals by measuring the light they emit in a flame. A solution such as potassium chloride is aspirated into the flame. The solvent evaporates first. The remaining salt becomes dehydrated and then dissociates into free gaseous atoms in the ground state. Some of these atoms absorb energy from the flame and move to an excited state. When they return to the ground state, they emit photons at characteristic wavelengths. These emissions are very narrow...

key terms and concepts

Learn how atomic emission spectroscopy uses emitted light to identify elements, compare ICP-AES and ICP-OES, and measure samples with calibration curves.

Atomic Emission Spectroscopy for Element Analysis | JoVE K12

analytical chemistry

JoVE Core Analytical Chemistry simplifies complex chemical principles by breaking them down into clear, engaging animations, making topics from SI Units to NMR spectroscopy more accessible and straightforward. Additionally, the scientist-in-action videos highlight the application of these concepts in real-world research conducted in laboratories globally.

Louisiana Student Standards for Science

High School

Earth Science

Earth’s Place In The Universe

HS-ESS1-2

Chemistry

motion-and-stability-forces-and-interactions

Motion And Stability: Forces And Interactions

HS-PS2-6

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South Carolina College and Career Ready Science Standards

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Waves and Their Applications in Technologies for Information Transfer

C-PS4-4

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Students who demonstrate understanding can develop a model based on evidence to illustrate the life span of the sun and the role of nuclear fusion in the sun's core to release energy in the form of radiation.  Clarification Statement: Emphasis is on the energy transfer mechanisms that allow energy from nuclear fusion in the sun's core to reach Earth.  Examples of evidence for the model include observations of the masses and lifetimes of other stars, as well as the ways that the sun's radiation varies due to sudden solar flares ("space weather"), the 11-year sunspot cycle, and non-cyclic variations over centuries.  Assessment Boundary: Assessment does not include details of the atomic and sub-atomic processes involved with the sun's nuclear fusion.

3.3.9-12.A

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Nuclear Binding Energy

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Metal Flame Emission

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Atomic Emission Spectroscopy: Instrumentation

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Atomic Absorption Spectroscopy: Radiation and Light Sources

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Students who demonstrate understanding can construct an explanation of the Big Bang theory based on astronomical evidence of light spectra, motion of distant galaxies, and composition of matter in the universe.  Clarification Statement: Emphasis is on the astronomical evidence of the red shift of light from galaxies as an indication that the universe is currently expanding, the cosmic microwave background as the remnant radiation from the Big Bang, and the observed composition of ordinary matter of the universe, primarily found in stars and interstellar gases (from the spectra of electromagnetic radiation from stars), which matches that predicted by the Big Bang theory (3/4 hydrogen and 1/4 helium).  Assessment Boundary:

3.3.9-12.B

Spectrophotometry: Introduction

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Atomic Emission Spectroscopy: Lab

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Flame Photometry: Overview

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3.3.9-12.D

Atomic Emission Spectroscopy for Element Analysis

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