how new spectrometer technologies substantially …...how new spectrometer technologies...
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How new spectrometer technologies substantially cut operating costs
Introduction
Inductively coupled plasma optical emission spectrometry (ICP-OES) is routinely used for elemental analysis by professionals in environ-mental, industrial, and academic laboratories worldwide. This fundamental spectroscopy technology analyzes everything from soil and sludge to water and wastewater, plus various industrial process materials. It helps ensure that governmental regulations are met, assists in environmental cleanup efforts, and supports industrial research and processes.
In evaluating which ICP-OES instrument to select for a given set of tasks, two differing emphases emerge. Many independent laboratories — especially those specializing in environmental contract work — naturally require an adequate level of performance, but in addition prioritize sensitivity and speed. Their prime concern: choosing an instrument that can maintain the
A WHITE PAPER FROMSPECTRO ANALYTICAL INSTRUMENTS
highest possible number of tests per shift. By contrast, other operations — including many industrial research laboratories — prioritize stability and analytical precision.
However, both groups agree on the importance of a common concern: controlling costs. This can be difficult, since most ICP-OES instruments presently on the market incur a variety of opera-tional and maintenance expenses, both obvious and hidden, that dramatically increase their total cost of ownership.
Fortunately, some newer enhancements to traditional spectrometer technologies reduce or eliminate these expenses. This report explores how engineering innovations can significantly reduce costs — enabling substantial savings while improving performance.
The trouble with traditional ICP-OES instruments
Many users report that several specific
technical features of most spectrometers
can cause considerable trouble
and expense.
In older instruments, these may require
inordinate spending on maintenance
and repairs. (Naturally, such problems
are magnified by subsequent down-
time, which itself further depresses the
bottom line.)
Even in newer spectrometers, if they’re
based on traditional technology, problems
may be persistent — and expensive. The
troubles can often be traced to inherent
weaknesses in the instruments’ design,
such as the ones discussed below.
The price of purging
Conventional ICP-OES instruments rely
on at least one costly consumable: a
constant supply of purge gas.
Certain often-analyzed elements
(including most or all nonmetals)
require measurements below 200
nanometers (nm) in the advanced UV
range. Unfortunately, conventional
designs are open to the environment,
so atmospheric air is present in their
optical paths. And lines below 180 nm
are strongly absorbed by the molecular
oxygen and water in that air.
So such instruments must purge air by
replacing it with argon or nitrogen gas.
2
Again unfortunately, purging sufficient
air from the optical path can take up to
2 hours after startup. Most laboratories
can’t afford to lose that much produc-
tivity. So to maintain system integrity,
they must fill and purge gas continually
— even when the system is not analyz-
ing samples. This “standby purging”
often consumes 1 liter (L) of expensive
gas per minute. Result: up to several
thousand dollars in purge gas waste and
expense each year.
Finally, this constant-fill/purge design
increases the chance that impurities in
the gas may contaminate components of
the optical system — requiring additional
pricey repairs.
The cost of cooling
Not surprisingly, plasmas generate quite
a bit of heat. To deal with this, traditional
ICP-OES systems require users to add
on an external cooling system.
Typically a water-based chiller, this
expensive, complicated component can
represent a significant headache. It may
well generate the largest volume of user
complaints about conventional spec-
trometer designs.
It adds unwelcome complexity to the
overall system. It’s often prone to inter-
nal leaks, which can cause the failure of
expensive instrument components such
as the plasma RF generator or load coil.
It can require frequent maintenance, and
serve as a disproportionate source of
system downtime.
Few such cooling systems outlast their
spectrometers. In fact, chillers often re-
quire early (and expensive) replacement.
Direct expenses may comprise the great-
est headaches of all. A hefty addition
to the spectrometer’s initial base price,
the separate chiller purchase may total
as much as $5,000. And energy costs
for this power-hungry component boost
utility bills for the life of the instrument.
The expense of instability and lower sensitivity
Its optical system is the heart of any
ICP-OES instrument. Conventional optics
still used in the majority of spectrome-
ters today utilize diffraction gratings of
the echelle type. (French for “ladder,” this
describes a particular grating pattern.)
Echelle-based instruments provide
adequate performance in varying
analytical situations. However, in a
number of not-uncommon applications,
echelle-based systems struggle and
fail to provide the levels of
performance necessary.
First, the way an echelle-based spec-
trometer processes spectral lines makes
it susceptible to interference when spec-
tra for certain elements present them-
selves too close together. Stray light
from reflections caused by the system’s
multiple optical components (see more
on this topic below) increases back-
ground radiation and affects sensitivity.
This stray light interference means that
echelle technology makes it harder to
3
satisfactorily analyze very line-rich ma-
trices, such as those encountered with
metals or some organics.
A second disadvantage is the echelle
systems’ strongly wavelength-dependent
resolution. They exhibit higher resolution
in the 200 nm range, but lower resolu-
tion above 300 nm. This makes working
with those line-rich metal matrices even
more challenging, and may require extra
processing — which adds even more
time, trouble, and expense.
For example, a user trying to utilize a
spectrometer with conventional optics
to analyze a sample of high-aluminum
soil finds it difficult to accurately mea-
sure the sample’s parts per billion levels
of lead. In an echelle-based system, the
lead analytical line at 220.3 nm is influ-
enced by the aluminum analytical line at
220.4 nm. A clever optical design allows
the use of the less influenced lead line at
168 nm.
In a third design shortcoming, optical
systems in all conventional echelle-
based ICP-OES spectrometers utilize
four to eight reflective/transmission
components (mirrors, prisms, cross-
dispersers, etc.). However, light
transmission is decreased at each
reflection/transmission. Most systems
have enhancements to try to com-
pensate for these losses, but they still
lose significant percentages of light —
enough in some cases to substantially
degrade sensitivity.
The problem becomes acute in the UV/
VUV spectral range below 190 nm,
leading to lower sensitivities for cer-
tain wavelengths and their respective
elements (aluminum at about 167 nm,
lead at 168, phosphorous at 177, sulfur
at 180, and so on).
Another challenge: echelle system
optics’ openness to the environment
requires expensive fill/purge gas supply
to replace ambient air, as already noted.
But it also negatively impacts measure-
ment stability. Any pressure change
in the ambient atmosphere is echoed
within the optical system, changing
the diffraction index of the optic atmo-
sphere. This leads to wavelength drift,
which may negatively influence recovery
of accurate results.
Finally, the limitations of echelle optics
may disadvantage a user’s selection
of plasma viewing options when pur-
chasing a spectrometer. Traditional
radial-view systems often can’t handle
trace concentration levels of a signifi-
cant number of elements. So the user
may be forced (instead, or also) to buy
higher-sensitivity axial or even dual-view
systems, even though these suffer from
lower stability and matrix compatibility,
while their added complexities demand
extra maintenance, cleaning, and cost.
4
It all adds up
Traditional spectrometers also suffer
from a few other problems.
Generators often aren’t powerful
enough to deliver the higher levels
of performance routinely needed in
real-world laboratories. For example, in
analytical situations requiring high plas-
ma loads, conventional spectrometers
can struggle (or fail) if challenged to
supply sufficient power when suddenly
switching matrices with different types
of samples. So sample throughput may
be effectively reduced.
These spectrometers’ overly complex
software and operational routines can
also require excessively long (and thus
expensive) learning curves and training.
Such delays can have a significantly
negative impact on laboratory or in-
dustrial process productivity. Also, the
design deficiencies noted above — and
others — can all appreciably increase
the chance of expensive errors.
When added up, all these hidden main-
tenance and operational expenses
can easily triple a user’s real cost
of ownership.
New designs and substantial savings
Fortunately, innovative engineering
improvements have eliminated these high-
priced spectroscopy headaches. Certain
systems can surpass conventional designs
to deliver consistent, rapid — and consid-
erably less expensive — results, day in
and day out.
Example: the SPECTROBLUE ICP-OES
analyzer from SPECTRO Analytical Instru-
ments. This powerful spectrometer contin-
ually sets new benchmarks for simplified
operation, low maintenance, and assured
affordability. Users report that its innova-
tive engineering overcomes the problems
detailed above, enabling the achievement
of high throughput — yet with drastically
lower costs of operation.
5
Eliminating purge gas consumption
The instrument’s innovative technology
improves on conventional spectrometer
design. A unique sealed optical system
abolishes the necessity for constant purg-
ing of argon or nitrogen. That means no
gas consumables cost or purging delays.
Instead, the system is permanently
argon-filled, recirculating gas through a
small purifier cartridge good for 2 years of
life. The user can start and stop the instru-
ment at will. So the spectrometer achieves
highly stable analytical results and excel-
lent low UV performance, right from the
beginning of a shift, without purge waiting
or delays at startup.
With an estimated 600 cubic meters of
purge gas saved per year, at current prices
a user of this technology may save $3800
annually in gas consumption alone.
OPI-AIR Interface
12 CCDs
PurifyingCartridgeUV-Plus
Na
Li
K
Grating3600 gr/mm165 - 285 nm
Grating1800 gr/mm285 - 470 nm
Avoiding external cooling
Improved spectrometer technology
eliminates the need to buy, install, pow-
er, and maintain a separate, external,
water-based cooling system.
Instead, the SPECTROBLUE analyzer
comes from a line of the only spectrom-
eters currently available that integrate in-
novative, patented air-cooled technology.
Simple in conception, this approach
generates inherently less need than
conventional designs for maintenance or
downtime. It saves the higher continuing
energy costs of water-based chillers. It
eliminates leaks and corrosion. It’s proven
less prone to breakdown. And it avoids
the need for expensive early replacement.
Attaining strong sensitivity and stability
In numerous analytical situations, in-
novations in optical technology affect
performance measures such as sensitiv-
ity and stability, which can also impact
operational costs.
6
Example: SPECTRO analyzer models such
as SPECTROBLUE utilize a unique optics
approach known as Optimized Rowland
Circle Alignment (ORCA polychroma-
tor) technology. (Here “Circle” describes
an optical arrangement with a concave
grating, optimized to limit the loss of light
during diffraction.)
Echelle optical systems utilizing charge-
coupled device/charge injection device
(CCD/CID) technologies were developed in
the 1990s, using two-dimensional sen-
sors as their foundation. By contrast, the
ORCA polychromator technique takes full
advantage of linear array detectors. This
spectrometer’s ORCA polychromator-based
optical system employs 15 linear CCD de-
tectors mounted into 2 hollow-section cast
shells to cover the wavelength range from
165 to 770 nm. It enables simultaneous cap-
ture of a sample’s complete spectrum with-
in 4 seconds. Prime ORCA polychromator
characteristics: sensitivity across a broader
spectral range, and excellent long-term
stability due to factors such as the absence
of any optics purging needs.
As mentioned earlier, the question of which
spectrometer type to buy can also be influ-
enced by the quality of a choice’s optics.
For example, in many industrial applica-
tions, users routinely encounter high con-
centrations of target elements. For this kind
of work, users often choose a higher-preci-
sion, lower-sensitivity radial-view model.
However, if these users sometimes
also encounter samples with trace-
level concentrations, their conventional
echelle-based radial-view system may
well prove inadequate. They must instead
choose a higher-sensitivity axial-view mod-
el. (Note that axial-based instruments bal-
ance their improved sensitivity with lower
precision, lower stability, and lower matrix
compatibility, while their greater complexi-
ty demands more maintenance and incurs
higher operating costs.) Or depending
on anticipated usage, they may select a
dual-view instrument that can provide both
capabilities. Either alternative means more
expense.
SPECTROBLUE may relieve the user
from having to make that choice. ORCA
polychromator-enabled optics gives it
unusually low detection limits that let even
its radial-view version handle many trace
analysis applications with sufficient sensi-
tivity (in addition to radial view’s inherent
high precision).
In all three SPECTROBLUE versions —
axial, radial, or twin-interface models
— ORCA polychromator optics create a
direct, high-luminance optical path that
limits light loss and “stray light” while max-
imizing spectral separation and information
throughput. These and other engineering
innovations improve sensitivity and stabili-
ty, allow the system to more easily process
line-rich spectra, boost measurement accu-
racy, and reduce expensive rework.
7
Achieving even more advantages
Innovative spectrometer technologies offer
other attractive benefits.
A robust generator design provides ample
power reserves, so it can handle extreme
plasma loads, and adapt to quickly changing
demands. Suppose the instrument is run-
ning a set of wastewater samples containing
roughly similar levels of organic materials.
If a sample suddenly appears that shows
much higher organics levels — causing a
higher plasma load — the system can han-
dle the change and make the measurement
without troublesome or costly delays.
The example system (SPECTROBLUE) also
uses a proprietary technology to enable
one-sample wavelength normalization. This
capability may be especially advantageous
for a large organization with many sites. It
can run the same methods on this same
model of analyzer at different locations —
using the same setup, without the need for
redundant local method development —
and get directly comparable results, with-
out costly delays. Larger operations can
standardize on a single model for uniform
results plus inventory cost savings.
Finally, innovative designs with less overall
instrument complexity result in easier,
less expensive installation, operation, and
maintenance. For just one instance, the
SPECTROBLUE approach is designed to
allow simple access and maintenance of
the introduction system. Software is intui-
tive and easy to learn. Overall, easy learn-
ing curves reduce training time and costs.
This is especially important where labora-
tories experience high operator turnover.
Conclusion
Traditional spectrometers bear the burden of a number of inherent problems in their
design. With more recent, more innovative technologies applied to improve ICP-OES
performance and usability in models such as SPECTROBLUE, users discover that many
headaches — and hefty costs — have been engineered out of the system.
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