High Resolution Continuum Source AAS
-Atomic Absorption Spectroscopy with
only one light source –
the only innovation of the XXI century
in Atomic Absorption and a new
challenge for Environmental Analysis
One light source for all elements Real multi element AAS
Simultaneous background correction Recording of reference spectra
More spectral information Wider working range
Better detection limits
HR-CS AAS - it´s something in between AAS and ICP OES !!
HR Continuum Source AAS –
HR-CS AAS
It is still routine AAS
1. Radiation source ⇒
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Xenon – short arc lamp/
HCL, EDL,
boosted HCL
2. Atomizer
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identical atomizer for flame technique
3. Monochromator ⇒
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High resolution /
low resolution
> 1:140000
1:10000
4. Detector
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CCD array detector/
single spot
detector (PMT)
5. Software
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Aspect CS/
WinAAS
To many limitations of traditional LS flame AAS
No flexibility , only defined lines
Less information - interferences, no vicinity
But
robustness, simple to operate, fastness, low costs
HR- CSAAS brings a new dimension of capabilities to AAS
All flame elements are permanently available from one source
Routine flame applications can be run as simple as in LS AAS
Detection limits are improved
All AAS correction modes are simultaneous and permanent
Additional sources of noise can be understood and corrected for
The method is not limited to atomic lines
Complex determinations due to spectral overlap can be corrected with
reference spectra
There is space for research in flame AAS
... – or basis of a new generation in atomic spectrometry
the HR-CS AAS?
The most important reasons to buy an contrAA !
1. SIMPLY THE BEST !!!
2. AAS with 1 Lamp only!
3. The total Flexibility! Flexibel and simple in one system!
4. Fastness! Immediately ready to measure!
5. Applications with complex sample matrix!
6. New dimension of information
7. Only Alternative to ICP
1. SIMPLY THE BEST !!!
The most innovative and state-of-the-art instrument in field
of AAS
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Prestige
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Status symbol! UNIQUE!
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Image of the customers
--
Global Players
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But also scientific image:
publications, research, projects...
contrAA 700
2. AAS with 1 Lamp only!
Replacement of
up to 60 different HCL´s
BGC lamp (deuterium lamp)
No lamp adjustment
No loss of energy with second light source
No loss of time regarding heating time of
the lamp
No problems with aging of the lamp
(line broadening, sensitivity loss...)
HR-CS AAS
Xenon short arc lamp as continuum radiator
ready for measuring:
- each element on - each wavelength
Comparison of intensity of different light sources
A Xenon-short arc lamp, XBO 301, 300 W, (GLE Berlin), „Hot - Spot“ - Mode B Xenon lamp, L 2479, 300 W, (HAMAMATSU), diffuse mode
C D2 - Lamp, MDO 620, 30 W, (HERAEUS)
Source: „High-resolution continuum source AAS“ Welz,Becker-Roß,Florek,Heitmann
2 0 0 2 5 0 3 0 0 3 5 0 4 0 0 1 E - 3 0 . 0 1 0 . 1 1 1 0 1 0 0 A B C R a d ia n c e [ W / c m 2 s r n m ] W a v e le n g t h [ n m ] Ag Au Pb Cd Pb Zn As
Lamp Cost
A Line source AAS needs a Deuterium Lamp and for each element a hollow cathode lamp
For some elements (e. g. As, Se ) most manufacturer recommend EDL`s or Superlamps
The contrAA needs only one lamp for background correction and all elements
550 D2 Lamp
2100 - 2200 Xenon lamp contrAA
1800 Power supply for superlamp
940 Superlamp
350 HCL (average)
Line Source AAS contrAA
3. The total Flexibility!
Flexibel and simple in one system!
No limitation of elements
No limitations of lines
Molecular bands and
Non metals (S,P...)
Minimum interferences
Simple to operate
seldom or rare requested analysed elements
exit window of HCL (UV or VIS permeable)
Cu - HCL ⇒ 217,9 nm, W - HCL ⇒ 255,1 nm
element interferences do not disturb the line selection atomic absorption using element lines or molecular bands
possible
analytical purpose decides element and line selection
Continuum source – provides more flexibility
All absorption and molecular lines are available
independent of:LS AAS use of most sensitive line
HR-CS AAS no limitations in line choice BUT:
Sometimes not the best SNR Non linear calibration curve
Use of less sensitive secundary lines No problems with interferences
all absorption lines are available
-independent if seldom or rare requested elements
Continuum source – provides more flexibility
Xenon lamp is covered in a safety lamp box
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provides emission spectrum of
the complete AAS relevant spectral
range (190 – 900 nm)
more flexibility…independent line choice
Gd in organic matrix as main component
Problem:
Extremly seldom, no standard application
High concentrated samples
No high concentrated standards available
No lamp available
all absorption lines are available
-independent if seldom or rare requested elements
Gd in organic matrix - all absorption lines are available
Gd 407.870 nm
Gd 368.4 nm
Standard calibration: 0.25 - 1.0 mg/ mL Gd
Continuum source – provides more flexibility
determination of
phosphorus
using PO – molecular bands
(e.g. 246,40 nm, 247,62 nm, 247,78 nm, 324,62 nm, 327,04 nm)
determination of
sulfur
using CS – molecular bands
(e.g. 257,59 nm, 258,06 nm)
determination of
fluorine
using AlF - molecular bands
(e.g. 227,47 nm)
determination of
chlorine
using AlCl or GaCl - molecular bands
(e.g. 261,44 nm, 249,06 nm)
absorption and molecular lines
for analytical use
Determination of P flame in defatting solvent 1-7 g/L P in C2H2/ air 7 pixel c0 = 0,29 g/L LOD = 22 mg/L 0,5 g/L P
Availability of molecular bands
PO- band at 324,619 nm C2H2/ air - flame
Determination of P flame in defatting solvent
Availability of molecular bands
Element Sample DF Concentration [g/L] RSD [%] P 324.619 nm Degreasing by boiling (A) 5 3.58 ±±±± 0.30 0.9 2 3.51 ±±±± 0.12 0.8 1 3.59 ±±±± 0.07 1.4 Degreasing by electricity (B) 5 5.61 ±±±± 0.29 0.9 2 5.46 ±±±± 0.13 2.4 1 4.92 ±±±± 0.07 0.8 (A) (B)
wine 1 C0 (g/L) 0,355 R2 0,9993 NWG (g/L) 0,071 Determination of S in wine wine 1+ 2000 ppm S
Availability of molecular bands
CS- band at 258,054 nm C2H2/ N2O - flame
Molecular bands could be used for determination of
elements which are normally not detectable with atomic absorption
sample DF S- conc.
[mg/L]
RSD [%]
Angelo Cremaschi 2003 Cabernet Merlot (13,5% Vol.)
1,043 155 9,2
Domaine de Gazel 2000 Minervois (12,0% Vol.)
1,043 165 7,6
Cabernet Sauvignon 2004 Récolte (12,0% Vol.)
1,043 148 11
Señorio del Aguila 1998 Reserva (13,0% Vol.)
1,043 288 11
Determination of S in wine
Simple….because it is a well known and well described
method!
New technique but not new!
Described methods(cookbook) are useable.
Comparable with other systems and results.
Simple analysis
4. Fastness
Of measurement
real sequential multi element analysis
Of method development and parameter optimization
you can see what you do!
Immediately ready to measure!
No delay time with flushing and rinsing the system
No delay with preheating time of lamps
Real Multielement Analysis
Single element method
-calibration Cu Pb Fe Ni Zn sample 1 sample 2 sample 3 …
LS AAS
calibration Cu Pb Fe Ni Zn sample 1 sample 2 sample 3 …CS AAS
Sequential multi element analysis
Schema ändern-sieht Varian zu ähnlich!!
Determination of 7 elements in high concentrated sugar
solution
Elements to be analyzed, Ca, Mg, Na, K, Cu, Fe and Pb
Elements are present in very different concentration ranges High sugar concentration leads to clogging of the burner head Elements require different sample preparation
Analysis very time consuming
Problems of a LS AAS user
All problems can be solved using CS AAS
Sample is used for fermentation purposes, dark brown very viscose solution
Sample preparation
LS AAS
Sample stock solution: 0.5 g sample + 2 mL HCl dilution up to 100 mL
Ca: 2 mL stock solution dilute with 0.1% KCl up to 50 mL
K: 0.5 mL stock solution dilute with 0.1% LaCl3 up to 100 mL
Mg: 2 mL stock solution dilute with 0.1% LaCl3 up to 50 mL
Fe: 10 mL stock solution dilute with 0.2% CaCl2 up to 50 mL
Na: 0.5 g sample + 2 mL HCl dilute with 0.1% KCl up to 50 mL
Pb: 0.5 g sample + 1 mL HCl dilute with 0.1% HNO3 up to 50 mL
Cu: 5.0 g sample + 2 mL HCl diluted up to 100 mL (Solution X) 10 mL solution X diluted with 1% HNO3 up to 50 mL
Sample preparation
CS AAS
Uniform sample preparation for all elements
Method parameter
Alternative wave lengths match to different element concentrations. Some wave lengths are not available with standard HCLs.
Method parameter
Different numbers of detectors (pixels) match to the element concentrations.
Multi element calibration
Pb 1-5 mg/L Na 5-20 mg/L
Mg 10-40 mg/L
Element spectrum
Ca Cu Fe
Multi element results
Element Concentration mg/kg RSD % Ca 4205 ± 38 1.2 Mg 1126 ± 18 0.4 K 74880 ± 288 0.2 Na 182 ± 6 0.7 Fe 179 ± 4 1.1 Cu 8.9 ± 0.1 0.4 Pb 0.82 ± 0.07 4.2Startup Time
The contrAA is ready to run samples within 5 minutes after the flame is ignited
Very fast analytical results Very low cost for gas
The ICP is ready to run samples 40 to 60 minutes after the plasma is ignited
It takes at least 40 minutes before you get the first analytical results The argon gas consumption is between 1200 and 1800 liter before you
5. Complicated applications_samples with
complex matrizes
Bernhard Welz, Departamento de Química, Universidade Federal de Santa Catarina, Florianópolis – SC, Brasil
In case of a spectral interference, we can see only the result, but not the reason –
therefore an optimization of parameters to avoid the spectral interferences is difficult.
LS AAS –
Visible is the Absorption vs. time within the small emission spectral range from the line source
Bernhard Welz, Departamento de Química, Universidade Federal de Santa Catarina, Florianópolis – SC, Brasil
Spectral information Graphite furnace - LS AAS
HR
HR--CS AAS CS AAS –– therethere isis a 3tha 3th DimensionDimension, , itit meansmeans wewe cancan seesee muchmuch more
more in in thethe background background
WeWe areare ableable to to seesee thethe reasonreason forfor thethe spectralspectral interferences interferences
WeWe cancan eliminateeliminate thethe spectralspectralinterferences
interferences
And And wewe havehave betterbetter possibilitiespossibilities to to correct correct the
Background correction par excellance
wavelength: 276.787 nm; sample: 10 µl i.e. 0.1 mg PACS-2 marine sediment SRM (NRC Canada); pyrolysis: 300°C; atomization: 1650°C; resolution ≈ 2 pm per pixel
before BB correction
after BB correction
(1. correction of broad-band effects)“true” analyte signal
before least-squares correction
wavelength: 276.787 nm; sample: 10 µl i.e. 0.1 mg PACS-2 marine sediment SRM (NRC Canada); pyrolysis: 300°C; atomization: 1650°C; resolution ≈ 2 pm per pixel
(2. correction of molecular background)
reference pixels
simultaneous
optical double beam
sequential lamp drift reference pixels reference spectrum simultaneous BG correction, sequential (D2 lamp,
Zeeman effect, reverse line method) unspecific absorption reference pixels simultaneous Lamp modulation sequential thermal emission Correction CS- AAS Correction LS- AAS Source of Error
What should be corrected ?
structured background
- spektral interferences with other atom lines
- moleculare absorptions
broad-band background
- streyligth from particels
- thermal emission
instrumental influences
- Intensity drift of light source
- thermal drift
- detector failer
Background Correction - simultaneously
- no loss of analysis time - spectral resolution
Effects are directly readable
- Structured background - Intensity drift
- Continuous weakening - Emission
Ni: 232,003 nm Fe: 232,036 nm Ni: 232,140 nm
Determination of Ni in grass flour
spectral band wide: 1,95 pm/ pixel spectral vicinity: 0,39 nm
Ni Fe
sample
Ni
Monochromator – minimization of spectral interferences
Warum misst man einmal mehr und manchmal weniger Bei diesen Störungen???
standard 0,4 mg/L Ni 5,0 mg/L Fe Ni: 232,003 nm Fe: 232,036 nm Ni: 232,140 nm
Determination of Ni in grass flour
sample
spectral interferences become visible but do not disturb the accuracy
background correction error with D2
Determination of Cu, Ni, Fe in galvanic bath
expected concentration: (r = 1,2 kg/L) Cu 30 – 40 g/Kg Ni 2 g/Kg
Fe 10 g/kg
Line selection defined by analytical task
Cu 244,164 nm Ni 231,234 nm Fe 303,739 nm dilution:
factor 200
+
spectral band wide: 2,1 pm/ pixel spectral vicinity: 0,11 nm
Cu: 324,754 nm Ni: 324,846 nm
Determination of Cu in Ni- galvanic bath
absorption CS AAS: 0,089 Abs absorption LS AAS: 0,057 Abs D2 – overcorrection: error -36%
More spectral information
about complex or unknown sample
6. New dimension of information
3dimensional information/Spectra
Information about the line vicinity
New dimension of information content
Int. wave length spectra Abs. wave length spectra 2D Abs. wave length spectra 3D
More information than LS AAS
- Easy method development - Results easy to evaluate
Detector – provides more information
UV- sensitive linear array detector (CCD)
„Back Thinned” CCD chip
High quantum efficiency High UV-sensitivity
588 pixel
each pixel as an individual detector
instead of:
exit slit for LS AAS
photomultiplier tube (PMT)
New detector technology for AAS
guarantees best signal to noise ratio
and more information content
Detector – provides more information
Hydride technique - advanced information content for transient
signals
As signal – 1 µg/L
continuous hydride mode
As
As
easy
error detectionimproves accuracy
eaier method development
Time resolved absorbance
Sample cup became empty
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Air molecular absorptionTime and wavelength resolved absorbance
7. Cost effective and only alternative to ICP
Costs – Time – Manpower – Experience!
No argon neccessary
Higher purchasing and maintance costs
Better experience necessary
Installation and Uptime
It takes 2 to 3 hours to install a Flame AAS! It takes 2 to 3 days to install an ICP-OES!
Uptime ( time between service calls) is much higher for an AAS instrument Compare the maintance costs ICP – AAS!
HR-CS AAS: Bridging the gap between AAS and ICP
combined withSpeed
Flexibility
Information
AAS
ICP
HR-CS AAS
Simplicity
Less interferences
Robustness
10. Method of choice for direct solid
sampling AAS
Strongest background correction
No influence of Magnetic field
Improved solid sampler
Key Application contrAA
Agriculture – soil extracts Electroplating solutions Clinical samples
Analysis of precious metal solutions Trace elements in Metals
As,Se in Cu or Co
Al in steel
Wear metals in oil Foodstuff
Additives in oil Etc.