Name: plasma sources in atomic emission spectroscopy
Uploaded: 2024-12-05T18:32:16.000Z
Duration: 1 min 29 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: Lab

ICP는 높은 안정성, 낮은 노이즈 및 정확한 실험 조건에서 간섭이 없기 때문에 AES에 선호되는 소스입니다.
일반적으로 용액 샘플을 분석합니다. 또한 고체 시료는 전열 기화 또는 레이저 및 스파크 제거를 통해 직접 분석됩니다.
플라즈마 방출 분광법은 주기율표에서 약 60개의 원소를 정성적으로 식별하고 정량화할 수 있습니다.
그러나 붕소, 탄소, 질소, 인 및 황과 같은 원소는 방출선이 180nm 미만으로 떨어지기 때문에 대기 구성 요소의 간섭을 유발하기 때문에 진공 분광계가 필요합니다.
알칼리 금속 검출은 부적절한 작동 조건과 근적외선 방출선으로 인해 문제가 발생합니다.
플라즈마 방출 분광법에서 검량선(calibration curve)은 분석물 농도에 대한 라인 강도에 비례하는 전기 신호의 선형 플롯입니다.
정량 분석의 경우, 외부 표준물질 또는 내부 표준물질(분석물과 유사한 방출선 및 화학적 간섭을 가진)이 일반적으로 사용됩니다.
그러나 여기 소스 온도 및 분무 효율과 같은 요인이 제어 할 수없는 방출 강도에 영향을 미치는 경우 내부 표준이 선호됩니다.

원자 방출 분광학: 연구실

원자 방출 분광학: (AES)는 강력한 분석 기법으로, 특히 플라즈마 소스와 함께 사용할 때 효과적이며 특징적인 방출선에서 풍부한 스펙트럼을 생성합니다. 특히 ICP(유도 결합 플라즈마)는 최적의 실험 조건에서 높은 안정성, 낮은 소음, 낮은 배경 및 최소한의 간섭으로 인해 우수한 정량 분석 ​​자료를 생성합니다. 그러나 새로운 공기 작동식 마이크로파 소스가 기존 ICP 소스보다 비용 효율적일 수 있는 유망한 대안으로 떠오르고 있습니다. AES는 주로 액체 샘플을 분석하는 데 사용됩니다. 그러나 플라즈마 방출은 또한 전열 기화, 레이저 및 스파크 절제, 글로우 방전 기화와 같은 다양한 절차를 통해 달성할 수 있는 고체 시료의 직접적인 분석을 허용합니다.

이론적으로 모든 금속 원소는 플라즈마 방출 분광법으로 측정할 수 있습니다. 알칼리 금속에 대한 이 방법의 효과는 까다로운 작동 조건과 근적외선 영역의 두드러진 스펙트럼 선 배치로 인해 제한됩니다. 이로 인해 주로 자외선 복사용으로 설계된 많은 플라즈마 분광기에서 검출 문제가 발생할 수 있습니다. 결과적으로 플라즈마 방출 분광법은 일반적으로 약 60개의 원소를 측정하는 것으로 제한됩니다. 대부분의 요소에는 식별 및 정량화에 적합한 몇 가지 눈에 띄는 선이 있습니다. 따라서 일반적으로 모든 원소를 결정하기 위한 적합한 선을 식별할 수 있습니다. 선의 선택은 표본에 존재할 수 있는 다른 원소를 평가하는 데 달려 있습니다. 관심 원소에 대한 선 선택 중에 다른 원소의 선이 겹치는 것을 피해야 합니다.

플라즈마 소스는 종종 선형 교정 곡선을 생성하지만 자체 흡수, 잘못된 배경 보정, 이온화 ​​및 검출 시스템의 비선형 반응과 같은 요인으로 인해 선형성에서 벗어날 수 있습니다. 가능하다면 외부 표준을 사용하여 정량 분석을 수행하는 것이 가장 좋습니다. 그러나 여기 소스의 온도 및 원자화 효율을 포함하여 많은 매개변수가 방출 강도에 큰 영향을 미칠 수 있습니다. 소스 매개변수의 변화를 제어하기 어려운 경우 내부 표준을 사용할 수 있습니다.

AES는 강력한 분석 기법으로, 플라즈마 소스와 함께 사용할 때 특히 효과적이며 특성 방출 라인에서 풍부한 스펙트럼을 생성합니다. ...

Education

교육

JoVE Core

Analytical Chemistry

분석 화학

Unit 1

제1단원

Atomic Spectroscopy

원자 분광법

KEY TERMS AND CONCEPTS

주요 용어 및 개념

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 emission spectroscopy is mainly used for liquid samples, but plasma emission can also be used for solid samples. Direct solid analysis can be done with electrothermal vaporization, laser and spark ablation, or glow-discharge vaporization.

In theory, plasma emission spectrometry can determine all metallic elements. In practice, its use for alkali metals is limited. Their strong spectral lines are in the near-infrared region, which can be hard to detect in many instruments made mainly for ultraviolet light. Because of this, plasma emission spectroscopy is usually used for about 60 elements.

Most elements have several strong lines that can help with both identification and measurement. A good line is usually chosen by checking overlap with lines from other elements in the sample. Plasma sources often give linear calibration curves, but some curves can deviate from linearity. This can happen because of self-absorption, background correction errors, ionization, or detector response problems.

When possible, quantitative analysis is best done with external standards. These are known samples used to compare emission intensity. Emission intensity can also change with source temperature and atomization efficiency, which is how well a sample turns into atoms. When source conditions are hard to keep constant, internal standards can help improve the measurement.

Plasma Sources in Atomic Emission Spectroscopy

plasma-sources-in-atomic-emission-spectroscopy

atomic spectroscopy: absorption, emission, and fluorescence

atomic-spectroscopy-absorption-emission-and-fluorescence

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

atomic-spectroscopy-effects-of-temperature

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

atomic-absorption-spectroscopy-instrumentation

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

atomic-absorption-spectroscopy-radiation-and-light-sources

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

atomic-absorption-spectroscopy-atomization-methods

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

atomic-absorption-spectroscopy-interference

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 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,...

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

inductively-coupled-plasma-atomic-emission-spectroscopy-principle

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

inductively-coupled-plasma-atomic-emission-spectroscopy

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

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 plasma sources improve atomic emission spectroscopy, from ICP analysis to solid sample methods, calibration, and internal standards.

Plasma Sources in Atomic Emission Spectroscopy | 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

Texas Essential Knowledge and Skills

Physics

PHYS.8

PHYS.8.F

south-carolina-college-and-career-ready-science-standards

South Carolina College and Career Ready Science Standards

waves-and-their-applications-in-technologies-for-information-transfer

Waves and Their Applications in Technologies for Information Transfer

C-PS4-4

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Atomic Structure

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Nuclear Stability

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3.3.9-12.A

Emission Spectra

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Atomic Spectroscopy: Absorption, Emission, and Fluorescence

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Space-Time Curvature and the General Theory of Relativity

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Nuclear Binding Energy

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Metal Flame Emission

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Molecular Spectroscopy: Absorption and 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: Overview

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3.3.9-12.D

Plasma Sources in Atomic Emission Spectroscopy

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