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Florida State University Libraries Electronic Theses, Treatises and Dissertations The Graduate School 2013 Accurate and Precise Determination of Low Concentration Iron, Arsenic, Selenium, Cadmium, and Other Trace Elements in Natural Samples by Octopole Collision/ Reaction Cell (CRC) Equipped Quadrupole- ICP-Ms Angela Dial Follow this and additional works at the FSU Digital Library. For more information, please contact [email protected]

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Florida State University Libraries

Electronic Theses, Treatises and Dissertations The Graduate School

2013

Accurate and Precise Determination of LowConcentration Iron, Arsenic, Selenium,Cadmium, and Other Trace Elements inNatural Samples by Octopole Collision/Reaction Cell (CRC) Equipped Quadrupole-ICP-MsAngela Dial

Follow this and additional works at the FSU Digital Library. For more information, please contact [email protected]

THE FLORIDA STATE UNIVERSITY

COLLEGE OF ARTS AND SCIENCES

ACCURATE AND PRECISE DETERMINATION OF LOW CONCENTRATION IRON,

ARSENIC, SELENIUM, CADMIUM, AND OTHER TRACE ELEMENTS IN NATURAL

SAMPLES BY OCTOPOLE COLLISION/REACTION CELL (CRC) EQUIPPED

QUADRUPOLE-ICP-MS

By

ANGELA DIAL

A Thesis submitted to the

Department of Earth, Ocean, and Atmospheric Science

in partial fulfillment of the

requirements for the degree of

Master of Science

Degree Awarded:

Spring Semester, 2013

ii

Angela Dial defended this thesis on March 28, 2013.

The members of the supervisory committee were:

William M. Landing

Professor Directing Thesis

Vincent J. M. Salters

Committee Member

Munir Humayun

Committee Member

The Graduate School has verified and approved the above-named committee members, and

certifies that the thesis has been approved in accordance with university requirements.

iii

TABLE OF CONTENTS

List of Tables ................................................................................................................................. iv

List of Figures ..................................................................................................................................v

Abstract ....................................................................................................................................... vi

1. INTRODUCTION .......................................................................................................................1

2. EXPERIMENTAL METHODS ...................................................................................................6

2.1 Reagents, Standards, and Sample Matrix .........................................................................6

2.2 Mass Spectrometry ...........................................................................................................6

2.2.1 Quadrupole-ICP-MS ..............................................................................................6

2.2.2 High Resolution-ICP-MS .......................................................................................8

3. RESULTS AND DISCUSSION ................................................................................................12

3.1 Analytical Figures of Merit .............................................................................................12

3.2 Plasma-based Interferences .............................................................................................16

3.3 Matrix-based Interferences ..............................................................................................20

3.4 Long-term Reproducibility ..............................................................................................24

4. CONCLUSIONS .......................................................................................................................26

REFERENCES ..............................................................................................................................27

BIOGRAPHICAL SKETCH .........................................................................................................30

iv

LIST OF TABLES

1. Plasma and matrix based polyatomic interferences on analytes of interest in their respective

matrix and sample type ............................................................................................................2

2. Instrumental settings of Q-ICP-MS (Agilent® 7500cs) for hot plasma and cool plasma

operations with collision – reaction cell ..................................................................................7

3. Instrumental settings of HR-ICP-MS (Thermo Finnigan® ElementXR) for low and medium

resolution Fe analyses ............................................................................................................11

4. Comparison of 56

Fe matrix blanks (in HNO3 matrix), sensitivity ([Fe]analyte = 1 µg/L; High

Purity Standard), and signal-to-noise (sensitivity/matrix blank) ratios of HR-ICP-MS

(Thermo Finnigan® ElementXR; University of Cambridge) and Q-ICP-MS (Agilent®

7500cs; Florida State University) ..........................................................................................12

5. Analytical figures of merit: sensitivity (cps/µg·L-1

per isotope), limit of detection (LoD, 3σ;

ng/L), and signal-to-noise ratios (S/N) of analytes of interest (51

V, 52

Cr, 55

Mn, 56

Fe, 57

Fe,

58

Ni, 59

Co, 63

Cu, 66

Zn, 75

As, 78

Se, 80

Se, 111

Cd, and 208

Pb) in hot and cool plasma conditions

with reaction mode or collision-reaction mode of CRC operation ........................................13

6. SRM NIST 1643e (Standard Reference Material - trace elements in freshwater) Fe and Cd

concentration data collected over a period of 7 months (Figure 11) .....................................25

v

LIST OF FIGURES

1. HR-ICP-MS (Thermo Finnigan® ElementXR) mass spectra of a 500 µg/L Fe standard

solution in 0.1 M HNO3 in low-resolution (m/∆m = 300) (Fig. 1.A) and medium-resolution

(m/∆m = 4000) (Fig. 1.B) mode ..............................................................................................3

2. Working principle of the Octopole Collision/Reaction Cell in collision and reaction

mode, adapted from the Agilent® 7500cs Operator’s Manual ...............................................5

3. Collision mode (CM) gas flow (He) optimization for 56

Fe (3.A), 78

Se (3.B), and 75

As (3.C) in

hot plasma ................................................................................................................................9

4. Reaction mode (RM) gas flow (H2) optimization for 56

Fe (4.A), 78

Se (4.B), and 75

As (4.C) in

hot plasma ..............................................................................................................................10

5. Comparison of air blank, matrix blank (0.44 M HNO3) and limit of detection (LoD: 3σ) of Fe

in hot and cool plasma mode (red and blue bars, respectively), with and without CRC

operation in RM .....................................................................................................................17

6. Comparison of sensitivities (cps/1 µg·L-1

) and matrix blanks (cps) for 56

Fe (6.A), 75

As (6.C),

78

Se (6.E), and 111

Cd (6.G) in all operating conditions: hot and cool plasma, Reaction Mode

(RM, H2 = 4.7 mL/min) and Collision-and-Reaction Mode (CRM, He = 2.8 mL/min and H2

= 2.0 mL/min) ........................................................................................................................18

7. Standard calibration in 0.44 M HNO3 of 56

Fe (circles with solid lines, y1-axis) and 57

Fe

(squares with dashed lines, y2-axis) operated under hot plasma (red) and cool plasma (blue)

conditions with the CRC in RM (H2 = 4.7 mL/min) .............................................................20

8. 75

As standard calibration in mixed acid (0.048 M HNO3 + 0.045 M HCl) operated under hot

plasma (red) and cool plasma (blue) conditions, with RM (H2 = 4.7 mL/min, circles solid

lines) and CRM (He = 2.8 mL/min and H2 = 2.0 mL/min, squares with dashed lines)

employed ...............................................................................................................................21

9. 95

Mo standard calibration (circles) in 0.44 M HNO3 executed in hot plasma with CRM (He =

3.0 mL/min and H2 = 2.0 mL/min), hot plasma with RM (H2 = 4.7 mL/min), cool plasma

with CRM (He = 2.8 mL/min and H2 = 2.0 mL/min), and cool plasma with RM (H2 =4.8

mL/min) .................................................................................................................................22

10. Comparison of sensitivity calibrations (slopes, cps/µg·L-1

) from a 111

Cd standard in 0.44 M

HNO3, operated in hot and cool plasma (red and blue bars, respectively) with the CRC in

CRM and RM (white and gray regions, respectively) ...........................................................23

11. SRM NIST 1643e (Standard Reference Material - trace elements in freshwater) Fe and Cd

concentration data collected over a period of 7 months ........................................................24

vi

ABSTRACT

An improved method for accurate and precise determination of trace quantity dissolved

metals and metalloids in natural samples by Octopole Collision/Reaction Cell (CRC) equipped

Quadrupole-Inductively Coupled Plasma-Mass Spectrometry (Agilent® 7500cs) is reported. Our

method is optimized for rapid analyses of small volume samples (~250 µL) in a variety of

matrices containing HNO3 and/or HCl. The present study focuses on elements with ICP-MS

plasma- and/or matrix based interferences, in particular 56

Fe (40

Ar16

O+),

75As (

40Ar

35Cl

+),

78Se

(40

Ar38

Ar+), and

111Cd (

95Mo

16O

+). We demonstrate efficient elimination of these polyatomic

interferences via the use of CRC in Reaction Mode (RM; H2 gas) and in Collision-Reaction

Mode (CRM; H2 and He gas). In addition, the efficiency of the instrument was evaluated under

both hot plasma (RF power 1500 Watts) and cool plasma (600 W) conditions. The present

method is optimized to analyze elements with large mass spectrometric interferences at sub parts

per billion level concentrations in a variety of natural samples and matrix compositions. We

report an average external precision of ≤ ~10% for minor (≤ 10 µg·L-1

) elements measured in a

1:100 dilution of NIST 1643e under two different plasma conditions and CRC operational

modes. Our measured concentration values for elements like Fe (99.6 µg/L), Mg (8020 µg/L),

Co (26.99 µg/L), Ni (62.54 µg/L), Cd (7.68 µg/L), Sb (59.6 µg/L), and Pb (19.82 µg/L) with a

large dynamic spread in concentrations in NIST 1643e are within ±12% to ±2% of the accepted /

published values.

1

CHAPTER 1

INTRODUCTION

Accurate and precise determination of trace metals in natural samples is essential to

discern their source, distribution, and role in the environment. Furthermore, this knowledge is

necessary to comprehend the natural biogeochemical cycles of these metals and potential

changes in their natural distribution caused by anthropogenic impacts. The role of transition

metals, such as Mn, Fe, Co, Cu, Ni, Zn, and Cd, as micronutrients in aqueous environments

generates a significant interest in understanding the biogeochemical cycle of these metals in

seawater (Brand et al, 1983; Boyd et al, 2000; Saito et al, 2005; Peers et al, 2005; Coale and

Bruland, 1988; Jones and Murray, 1984; Shaked et al, 2006; Cullen et al, 1999). Iron is of

special interest since it is a limiting factor in biological productivity throughout the world’s

oceans, particularly in high-nutrient low-chlorophyll regions (Johnson et al, 1997). Another

element of interest is Cr, as Cr has variable effects on biological cycles depending on its

oxidation state: chromium (III) is an essential nutrient for many organisms, however chromium

(VI) is highly toxic (Mertz, 1993; Kotaś and Stasicka, 1999). Another application for trace

element studies is the use of metals and metalloids like V, Zn, As, Se, Sb, and Pb as tracers of

anthropogenic pollution (Bruland et al, 1974; Plant et al, 2006; Callender, 2006). Accurate

documentation of these trace elements in the environment is imperative to aid in understanding

how biogeochemical cycles in natural systems operate and how they have been perturbed by

human activity.

Advances in inductively coupled plasma mass spectrometry (ICP-MS) over the past

decade have made it a popular analytical tool for rapid and simultaneous analyses of multiple

elements. However, accurate measurements of trace quantity dissolved metals and metalloids in

natural samples using ICP-MS is limited by the low concentration of elements in samples of

interests; contamination during sample collection, handling, and storage; and sample matrix-

based and ICP-MS plasma-based (mass spectrometer) isobaric and polyatomic interferences.

Moreover, a high first ionization potential (IP-1), volatility in analyte matrix, and surface

adsorption properties of an analyte can further compound the problems by diminishing

sensitivity and increasing the carry over effect between samples (Gaboardi & Humayun, 2009).

2

These analytical challenges are exacerbated with certain trace elements, such as Fe, As, Se, and

Cd, which have plasma- and/or matrix-based polyatomic and/or multiple charged mass

interferences on the major isotopes of the analyte. A representative list of elements of interest

and their major mass interferences from plasma and matrix sources are presented in Table 1.

Isobaric interferences are generally due to Ar, O2, N2, and C based polyatomic molecules

(plasma-based) or metal oxides (matrix-based), which have similar mass-to-charge (m/z) ratios

as the analyte. Additionally, the nature of the sample matrix (complex or simple) can play

important roles in formation of polyatomic interferences. For example, elements like V, Cr, and

As all have Cl-based interferences in the presence of HCl in the matrix (Table 1). In the present

study, rain water samples are analyzed in “dilute aqua regia” (0.048 M HNO3 + 0.045 M HCl)

for stabilization of dissolved trace metals as well as volatile mercury (Landing et al, 1998), a

strategy that increases the range of possible interferences due to chlorine based polyatomic ion

formation.

Table 1. Plasma and matrix based polyatomic interferences on analytes of interest in their

respective matrix and sample type.

 

Analyte Plasma

Interference

Matrix

Interference Sample Application

51V

 

35Cl

16O

+ Rainwater

52Cr

40Ar

12C

+

35Cl

16O

1H

+ Rainwater

55Mn

Seawater/Rainwater

56Fe

40Ar

16O

+

Seawater/Rainwater

57Fe

40Ar

16O

1H

+

Seawater/Rainwater

58Ni

Seawater/Rainwater

59Co

Seawater/Rainwater

63Cu

Seawater/Rainwater

66Zn

Seawater/Rainwater

75As

 

40Ar

35Cl

+ Rainwater

78Se

40Ar

38Ar

+

Rainwater

80Se

40Ar

40Ar

+

 Rainwater

111Cd

95

Mo16

O+ Seawater/Rainwater

208Pb

Seawater/Rainwater

3

The success of ICP-MS analyses depends on the ability to overcome matrix- and plasma-

based isobaric, polyatomic, and multiple charged interferences on an analyte. High Resolution-

ICP-MS (HR-ICP-MS) is able to resolve many elements from their mass interferences using a

higher mass resolution defined as the resolving power:

!!"#$% =  !

∆! 

where m is the analyte’s mass (at 100% peak height) and Δm is the mass difference between the

analyte and interferent peaks (Weyer and Schweiters, 2003). However, HR-ICP-MS methods are

unsuitable for measurements of mass limited samples due to significant decreases in sensitivity

in mass resolution modes (m/Δm) of 2000 or higher. Figure 1 exemplifies this decrease in 56

Fe

sensitivity with increase in mass resolution. For analyses in medium resolution (m/Δm = 4000),

sensitivity is reduced by a factor of 25 from that of low resolution (m/Δm = 300). A Quadrupole-

ICP-MS (Q-ICP-MS) is incapable of resolving analyte peaks from any interference’s using

higher mass resolutions, however a Q-ICP-MS equipped with Collision/Reaction Cell (CRC) can

effectively eliminate the interfering polyatomic molecules by capitalizing on their bigger

collision radius and using energy discrimination (Tanner et al, 2002; Iglesias et al, 2002;

Leonhard et al, 2002; McCurdy & Woods, 2004).

Figure 1. HR-ICP-MS (Thermo Finnigan® ElementXR) mass spectra of a 500 µg/L Fe standard

solution in 0.1 M HNO3 in low-resolution (m/∆m = 300) (Fig. 1.A) and medium-resolution

(m/∆m = 4000) (Fig. 1.B) mode. In low-resolution (Faraday ion detection) the 56

Fe (55.9349

amu) peak is dominated by 40

Ar16

O+ (55.9573 amu) interference. In medium-resolution (Analog

ion detection) a complete peak separation between 56

Fe+ (left) from

40Ar

16O

+ (right) is achieved.

However, there is an order of magnitude decrease in overall sensitivity from low resolution

(56

Fe+ +

40Ar

16O

+ = 1.8 x 10

9) to medium resolution (

56Fe

+ = 1.0 x 10

8,

40Ar

16O

+ = 1.0 x 10

8).

4

In this study, we present an improved method of accurate and precise concentration

determination of elements with plasma- and/or matrix-based polyatomic mass spectrometric

interferences via utilization of an Agilent® 7500cs Q-ICP-MS equipped with an Octopole CRC.

The CRC is an off-axis chamber, 2 mL in volume, with a positive potential bias along the ion

flow path. The CRC can be flooded with low molecular weight gases, such as H2 (reaction mode)

and/or He (collision mode), which can collide with the passing ions of the analyte. Polyatomic

interferences have a larger collision cross section than monatomic analytes of interest, therefore

increasing the collision frequency of the interferent with the H2 and/or He molecules in the CRC.

The choice of gas determines whether the CRC is operated under reaction mode and/or collision

mode. In reaction mode, H2 gas eliminates interferences in two ways: a. by charge transfer –

polyatomic interferent molecules collide with H2 and transfer its charge to the H2 molecule, thus

making it mute to the SEM detector; and b. by mass transfer – the polyatomic interferent reacts

with H2 and bonds with one hydrogen atom, increasing its mass by 1 amu (Figure 2a). In

collision mode, He eliminates interferences by colliding with polyatomic molecules and reducing

their kinetic energy through energy transfer from the interferent to He. This drop in kinetic

energy coupled with the positive energy discrimination of the CRC stops the interferent from

traversing the cell (Figure 2b). This method of energy bias against the polyatomic interferent is

termed kinetic energy discrimination (KED).

In addition to utilizing the Octopole Collision/Reaction Cell to reduce interferences, we

optimized the instrument under hot plasma (1500 Watts) and cool plasma (600 W) conditions.

The cool plasma (~6000 K) reduces the ionization efficiency of elements with high IP-1 (e.g.,

High IP-1: Ar = 15.76 eV and As = 9.81 eV) as compared to hot plasma (~8000 K) conditions. In

the present study, we document the elimination of plasma- and matrix-based polyatomic

interferences with different plasma and CRC settings.

5

Figure 2. Working principle of the Octopole Collision/Reaction Cell in collision and reaction

mode, adapted from the Agilent® 7500cs Operator’s Manual. Polyatomic interference

elimination by charge transfer and atom transfer reactions (reaction mode) are shown in Fig. 2.A.

During atom transfer reactions, the polyatomic mass interferent (40

Ar16

O+) reacts with H2

(reaction gas) and binds one hydrogen atom to the interferent, increasing its mass by one amu.

During charge transfer reactions, the polyatomic interferent transfers its charge to a H2 molecule,

thus becoming mute to the SEM detector. Interference elimination in collision mode, utilizing an

inert gas like He (collision gas), is shown in Fig. 2.B. Polyatomic interferences (40

Ar16

O+) have a

larger ionic radius (effective nuclear volume) than the monatomic analyte of interest (56

Fe),

increasing the collision frequency of the interferent over that of the analyte with the collision gas

(He). More collisions of the interferent leads to greater loss of kinetic energy for the interferent

compared to the monatomic analyte of the same mass. This kinetic energy discrimination against

larger polyatomic interferences stops it from traversing the off-axis CRC. Moreover, in collision

mode, dissociation of polyatomic interferences upon collision with cell gas (He) also eliminates

interference.

Fig. 2A.

Fig. 2B.

6

CHAPTER 2

EXPERIMENTAL METHODS

2.1 Reagents, Standards, and Sample Matrix

All acids, ICP-MS standards, and samples were prepared using 18.3 MΩ·cm MQ water.

We used Optima® (Fisher®) grade nitric and hydrochloric acid for analyte matrix preparation.

Analyte blanks of the water source, acids, and elemental standards were closely monitored

throughout the entire experiment. Accurate molarity of each batch of acid was determined by

titrimetric methods. Samples were analyzed in three different acid matrixes: 0.44 M HNO3 for

general ICP-MS analysis; 1.0 M HNO3 for seawater samples prepared using the method from

Milne et al (2010); and mixed acid (0.048 M HNO3 + 0.045 M HCl) for measurements of trace

metals and mercury in rainwater samples using the method from Landing et al (1998). In

addition, all calibration standards were prepared gravimetrically from High Purity Standards

(HPS). Laboratory supplies used in the present body of work were acid cleaned using reagent

grade 8.0 M HNO3 at sub-boiling temperature.

2.2 Mass Spectrometry

2.2.1 Quadrupole-ICP-MS

Elemental concentrations were determined with an Agilent® 7500cs single collector

Quadrupole-ICP-MS equipped with an Octopole Collision / Reaction Cell (CRC). Depending on

the experiment, the instrument was operated either under hot plasma (1500 W) or cool plasma

(600 W) conditions. The sample introduction for both plasma conditions was done with a

nominal 100 µL/min self-aspirating concentric PFA nebulizer (ESITM

), a Scott-type quartz spray

chamber, a quartz torch with built-in quartz injector (2.5 mm i.d.), and nickel sampler and

skimmer cones. The key differences between the two plasma-operating conditions are the

voltage settings on Extraction lens 1 (EL-1) and Extraction lens 2 (EL-2). Under hot plasma

conditions, optimal sensitivity was achieved with a slightly positive voltage for EL-1 (3.5 to 4.0

V) and a negative voltage for EL-2 (-160 to -150 V). In cool plasma, optimal sensitivity was

obtained in “soft extraction” mode by applying a negative voltage on EL-1 (-180 to -175 V) and

a positive voltage on EL-2 (-5 to 5 V) (Table 2) (Misra & Froelich, 2009).

7

Table 2. Instrumental settings of Q-ICP-MS (Agilent® 7500cs) for hot plasma and cool plasma

operations with collision – reaction cell.

Instrumental Parameter Hot Plasma (1500 W) Cool Plasma (600 W)

Spray Chamber Quartz Quartz

Torch/Injector Quartz/Quartz Quartz/Quartz

Shield Torch Platinum Platinum

Sampler Cone Nickel Nickel

Skimmer Cone Nickel Nickel

Nebulizer ~100 µL/min Concentric (PFA) ~100 µL/min Concentric (PFA)

Spray Chamber Temperature 2 °C 2 °C

Carrier Gas Flow 0.70 to 0.75 L/min 0.60 to 0.65 L/min

Make-up Gas Flow 0.30 to 0.35 L/min 0.17 to 0.22 L/min

Sampling Depth 6.5 to 7.5 mm 7.0 to 8.0 mm

Extraction 1 Lens 3.5 to 4.0 V -180 to -175 V

Extraction 2 Lens -160 to -150 V -5 to 5 V

Reaction Cell H2 = 4.6 to 4.9 mL/min H2 = 4.6 to 4.9 mL/min

Gas Flows He = 0 mL/min He = 0 mL/min

Collision and Reaction H2 = 2.5 to 3.0 mL/min H2 = 2.5 to 3.0 mL/min

Cell Gas Flows He = 2.0 to 2.5 mL/min He = 2.0 to 2.5 mL/min

For daily operation, the ICP-MS was initially tuned under hot plasma (1500 W)

conditions with the CRC disabled. Instrumental sensitivity and stability (%RSD ≤ 1.5%) was

optimized for masses (m/z) 7Li

+,

24Mg

+,

59Co

+,

89Y

+,

140Ce

+, and

205Tl

+. To minimize the

formation of polyatomic interferences, the sampling depth and gas flows were adjusted to have

<2% oxide formation (m/z: 140

Ce16

O+/140

Ce+ or 156/140) and <2.5% doubly charged ion

formation (m/z: 140

Ce++

/140

Ce+

or 70/140). Tuning of the quadrupole (peak resolution, peak

shape, and resolution axis) and detector calibration (pulse to analog counting mode linearity)

were all performed via auto-tune. For cool plasma measurements, the instrument was first

optimized in hot plasma before lowering the forward RF power to 600 W. The instrument was

re-optimized in cool plasma after allowing the vacuum pressure to stabilize for ~15 minutes. In

both plasma modes, the CRC was operated by using H2 gas (reaction mode), He gas (collision

mode), or both He and H2 gas (collision-and-reaction mode). For the present study, only reaction

mode (RM) or collision-and-reaction mode (CRM) are discussed due to their greater efficiency

in reducing plasma- and matrix-based interferences (Feldmann et al, 1999; Iglesias et al, 2002;

8

Leonhard et al, 2002). The instrument under collision mode (CM) was not able to provide

acceptable signal-to-noise (S/N) ratios for several elements, in particular 56

Fe, 78

Se, and 75

As

(Figure 3 A-B). The best detection limit for an element results from a combination of both low

blanks and high sensitivity during ICP-MS measurement, represented as S/N in cps-per-µg·L-1

/

matrix blank.

To prolong the operational life of the Octopole CRC, the total H2 and/or He gas flows

under both RM and CRM were kept below 5.0 mL/min. This limits the total amount of H2 atoms

entering the cell, which minimizes the physical corrosion of the Octopole CRC over time. Daily

operational gas flows were chosen based on optimization of the S/N ratio for particular elements

in varying sample-types and matrices. A typical example of a gas flow optimization of the RM

(H2 only) on 56

Fe, 78

Se, and 75

As is given in Figure 4. Removal of interferences from 56

Fe is a

benchmark for CRC optimization due to the sheer magnitude of 40

Ar16

O+ interferences on

56Fe

+

(4A). For 56

Fe, ICP-MS operation without RM (H2 = 0 mL/min) has a background noise of ~91%

of the analyte signal (the 1 µg/L Fe standard and matrix blank sensitivities are ~46x106 cps and

~42x106cps, respectively). With an operational and optimized RM, the noise is reduced to ~3%

(130,000 cps and 4,000 cps, respectively) of analyte signal intensity. Moreover, the optimization

of gas flows on 56

Fe offers an excellent S/N for low concentration Fe determination, without

decreasing the S/N of other analytes of interest, such as 78

Se (Figure 4B) and 75

As (Figure 4C).

2.2.2 High Resolution-ICP-MS

A Thermo Finnigan® Element XR at the University of Cambridge was used to compare

the instrumental capabilities of an HR-ICP-MS with that of a Quadrupole-ICP-MS. The sample

introduction setup was as follows: quartz cyclonic spray chamber, platinum injector, platinum

sampler and skimmer cones, and a 50 µL/min Savillex C-Flow nebulizer. Measurements in low

resolution were made using Faraday counting and pulse mode, while measurements made in

medium resolution were performed under analog counting mode. All analyses were performed

after sensitivity optimization (~2.5 Mcps / µg·L-1

) on 115

In (Table 3).

9

Figure 3. Collision mode (CM) gas flow (He) optimization for

56Fe (3.A),

78Se (3.B), and

75As

(3.C) in hot plasma. The volume of He gas flow into the CRC (mL/min) is plotted on the X-axis;

the left hand Y-axis denotes analyte sensitivity in matrix blank and standard (1 µg/L) in

logarithmic scale; the right hand Y-axis denotes the signal-to-noise ratio (1 µg/L standard

sensitivity /matrix blank) in linear scale. Analyses were done in mixed acid matrix (0.048 M

HNO3 + 0.045 M HCl). Circles represent matrix blanks; squares: standard sensitivity; and

diamonds: signal-to-noise ratios (S/N). The ranges of optimal gas flow, as defined by low matrix

blank and high S/N, is shaded in gray. 56

Fe and 78

Se have plasma based Ar-O and Ar-Ar

interferences respectively, whereas, 75

As have matrix-based interference from Ar-Cl. Operation

of CRC in CM is inefficient in eliminating plasma-based polyatomic interferences, which is

evident from very low S/N (< 5) for 56

Fe and 78

Se at high He gas flow. For 75

As, a better S/N

(~25) can be achieved in CM as weaker Ar-Cl bonds are more efficiently broken during collision

with He. This inefficiency of CM in removing plasma based polyatomic interferences essentially

rules out analyses of elements with Ar based interference via this CRC mode.

10

Figure 4. Reaction mode (RM) gas flow (H2) optimization for 56

Fe (4.A), 78

Se (4.B), and 75

As

(4.C) in hot plasma. The volume of H2 gas flow into the CRC (mL/min) is plotted on the X-axis;

the left hand Y-axis denotes analyte sensitivity in matrix blank and standard (1 µg/L) in

logarithmic scale; the right hand Y-axis denotes the signal-to-noise ratio (1 µg/L standard

sensitivity /matrix blank) in linear scale. Analyses were done in mixed acid matrix (0.048 M

HNO3 + 0.045 M HCl). Circles represent matrix blanks; squares: standard sensitivity; and

diamonds: signal-to-noise ratios (S/N). The ranges of optimal gas flow, as defined by low matrix

blank and high S/N, is shaded in gray. Operation of CRC in RM is efficient in knocking out

plasma and matrix based polyatomic interferences as evident from high S/N (> 30) for 56

Fe, 78

Se

and 75

As at moderate H2 gas flow (4.5 ± 0.5 mL/min). Considering Fe (4.A), the sensitivity

difference between standard and matrix blank is ~9% (~ 46 x 106 cps and 42 x 10

6cps,

respectively) without the CRC in operation, whereas in RM with optimal gas flow, the difference

increases to ~97% (130,000 cps and 4,000 cps, respectively). Moreover, optimizing the CRC on 56

Fe in RM ensures that other analytes of interest (75

As, 78

Se, 111

Cd) had high (≥ 30) S/N. In

addition, during gas flow optimization the lowest acceptable gas flow is chosen to reduce the

amount of H2 gas entering the Octopole CRC, hence minimizing physical degradation of the

CRC.

11

Table 3. Instrumental settings of HR-ICP-MS (Thermo Finnigan® ElementXR) for low and

medium resolution Fe analyses.

     

Instrumental Parameter Setting

Spray Chamber Quartz (cyclonic)

Injector Platinum

Sampler Cone Platinum

Skimmer Cone Platinum

Nebulizer ~50 µL/min Savillex C-Flow

Cool Gas Flow 15 L/min

Sample Gas Flow 1.075 L/min

Auxiliary Gas Flow 1.30 L/min

Additional Gas Flow 0.225 L/min

Sampling Depth -2.20 mm

Extraction Lens -2000 V

Focus -950 V

X-Deflection 5.25 V

Y-Deflection 2.25 V

Shape 125 V

Quad 1 2.50 V

Quad 2 -4.50 V

Focus Quad -1.00 V

Filter Lens 0.00 V

12

CHAPTER 3

RESULTS AND DISCUSSION

3.1 Analytical Figures of Merit

Direct comparison of HR-ICP-MS and Q-ICP-MS in terms of their sensitivity,

instrumental blanks, and signal-to-noise ratios is limited by the unavailability of these results in

published works. In Table 4 we present a comparative study of 56

Fe figures of merit from the two

types of instruments. The HR-ICP-MS (Thermo Finnigan® Element XR) has high sensitivity

and a comparatively high instrumental blank, resulting in a low signal-to-noise ratio (S/NLow Res =

~1; S/NMed Res = 120). The Quadrupole-ICP-MS is an Agilent® 7500cs which yields a better

signal-to-noise ratio for 56

Fe while utilizing cool plasma and reaction mode (H2 gas only), thus

offering a very low detection limit (S/NCool Plasma, RM = 210).

Table 4. Comparison of 56

Fe matrix blanks (in HNO3 matrix), sensitivity ([Fe]analyte = 1 µg/L;

High Purity Standard), and signal-to-noise (sensitivity/matrix blank) ratios of HR-ICP-MS

(Thermo Finnigan® ElementXR; University of Cambridge) and Q-ICP-MS (Agilent® 7500cs;

Florida State University). Q-ICP-MS was operated under reaction mode (CRC with H2 gas) in

both hot plasma (1500 W) and cool plasma (600 W) conditions.

     

 

Instrument Resolution Plasma

Power Matrix Matrix Blanks

(cps) 1 ppb

(cps) Signal/Noise Thermo Finnigan

Element XR Low 1250 W 0.1 M HNO3 ~1x109 ~1x10

9 ~1 Thermo Finnigan

Element XR Medium 1250 W 0.1 M HNO3 6,000 700,000 120

Agilent 7500cs Low 1500 W 0.44 M HNO3 1,300 52,000 40

Agilent 7500cs Low 600 W 0.44 M HNO3 710 150,000 210

Sample analyses by Q-ICP-MS included a full-metal scan of 71 elements, ranging from

mass 7Li to

238U. The Q-ICP-MS was operated under hot and cool plasma conditions, utilizing

reaction mode or collision-and-reaction mode, and with samples in three different matrix

compositions (0.44 M HNO3, 1.0 M HNO3, and mixed acid (0.048 M HNO3 + 0.045 M HCl)).

Table 5 lists the sensitivity in counts-per-second per parts-per-billion (cps/µg·L-1

) per isotope,

limit of detection in parts-per-trillion (ng/L), and signal-to-noise ratio of the major analytes of

13

Table 5. Analytical figures of merit: sensitivity (cps/µg·L-1

per isotope), limit of detection (LoD,

3σ; ng/L), and signal-to-noise ratios (S/N) of analytes of interest (51

V, 52

Cr, 55

Mn, 56

Fe, 57

Fe, 58

Ni, 59

Co, 63

Cu, 66

Zn, 75

As, 78

Se, 80

Se, 111

Cd, and 208

Pb) in hot and cool plasma conditions with

reaction mode or collision-reaction mode of CRC operation. Experiments were conducted using

three different matrices: 0.44 M HNO3 (5.A); 1.0 M HNO3 (5.B); and mixed acid matrix (0.048

M HNO3 + 0.045 M HCl) (5.C). Reported sensitivities are corrected for the percent abundance of

isotope of choice. The isotopic abundance correction of sensitivity allows for a more meaningful

comparison of blanks and instrumental sensitivity for different elements. Table 5.B. compares

the expected minimum (Bruland, 1983; Donat & Bruland, 1995) of a concentrated (20-fold)

seawater sample (Milne et al, 2010) with the optimal LoD (shaded gray) for each element.

Table 5.A. 0.44 M HNO3

Hot Plasma Cool Plasma

Analyte

CRC

Gas

Sensitivity

(cps/µg·L-1

)

LoD

(ng/L) S/N

Sensitivity

(cps/µg·L-1

)

LoD

(ng/L) S/N

51V

H2 16,000 3.0 240 44,000 0.39 1000

He + H2 21,000 1.2 470 53,000 0.34 470

52Cr

H2 16,000 4.5 50 81,000 2.5 560

He + H2 29,000 4.3 55 130,000 4.8 325

55Mn

H2 75,000 3.0 220 190,000 0.95 320

He + H2 52,000 1.0 220 200,000 6.2 605

56Fe

H2 57,000 3.2 40 160,000 0.86 210

He + H2 46,000 3.9 20 170,000 13 75

57Fe

H2 59,000 77 2 170,000 21 10

He + H2 45,000 96 1 180,000 11 12

58Ni

H2 8,000 13 25 37,000 3.3 440

He + H2 15,000 23 40 59,000 2.7 175

59Co

H2 24,000 0.93 700 62,000 0.15 3300

He + H2 29,000 0.95 1000 89,000 0.58 1650

63Cu

H2 3,800 7.6 60 20,000 1.0 270

He + H2 16,000 5.8 50 59,000 7.8 90

66Zn

H2 27,000 6.0 180 30,000 1.9 260

He + H2 23,000 1.6 120 35,000 9.6 17

75As

H2 1,500 3.5 120 860 5.0 80

He + H2 2,600 4.1 180 1,100 4.4 50

78Se

H2 4,200 36 25 2,100 36 20

He + H2 5,000 32 25 2,000 35 17

80Se

H2 4,400 30 14 2,200 34 18

He + H2 5,200 38 5 2,000 74 2

111Cd

H2 100,000 0.62 1500 45,000 0.84 440

He + H2 86,000 0.35 1800 44,000 3.0 235

208Pb

H2 210,000 0.26 1900 97,000 0.35 1700

He + H2 210,000 0.72 1300 115,000 4.6 270

14

Table 5.B. 1.0 M HNO3

Hot Plasma Cool Plasma Expected

Seawater

Minimum

(ng/L) Analyte

CRC

Gas

Sensitivity

(cps/µg·L-1

)

LoD

(ng/L) S/N

Sensitivity

(cps/µg·L-1

)

LoD

(ng/L) S/N

51V

H2 20,000 4.5 90 56,000 1.8 400 23,400

He + H2 23,000 0.082 230 37,000 3.5 210

52Cr

H2 20,000 0.22 60 94,000 0.027 610 3,060

He + H2 31,000 0.19 60 110,000 2.4 255

55Mn

H2 93,000 1.2 140 200,000 1.5 200 81.5

He + H2 57,000 1.7 160 150,000 2.0 640

56Fe

H2 71,000 8.4 30 190,000 4.3 90 20.4

He + H2 50,000 15 20 110,000 7.2 45

57Fe

H2 72,000 94 2 180,000 15 9 ─

He + H2 41,406 135 2 110,000 64 13

58Ni

H2 10,000 3.3 20 38,000 1.1 250 2,040

He + H2 16,000 2.3 40 35,000 11 140

59Co

H2 30,000 0.42 700 67,000 0.14 2100 4.08

He + H2 31,000 0.92 800 57,000 0.42 1500

63Cu

H2 4,800 5.0 30 20,000 6.0 250 510

He + H2 16,000 2.3 50 36,000 42 50

66Zn

H2 28,000 0.50 150 25,000 1.4 170 102

He + H2 22,000 1.4 160 19,000 95 30

75As

H2 160,000 3.1 120 170,000 13 60 20,400

He + H2 170,000 1.9 160 180,000 20 50

78Se

H2 3,800 21 440 710 42 3300 510

He + H2 4,200 14 175 1,200 55 1650

80Se

H2 3,800 25 270 650 110 260 ─

He + H2 4,800 36 90 1,200 702 17

111Cd

H2 110,000 0.30 1300 41,000 0.36 440 1.02

He + H2 86,000 0.38 1900 26,000 3.3 220

208Pb

H2 250,000 0.023 2000 100,000 0.30 1600 5.09

He + H2 230,000 0.27 2200 100,000 0.56 1000

15

Table 5.C. Mixed Acid (0.048M HCl plus 0.045M HNO3)

   Hot Plasma Cool Plasma

Analyte CRC Gas

Sensitivity

(cps/µg·L-1

)

LoD

(ng/L) S/N

Sensitivity

(cps/µg·L-1

)

LoD

(ng/L) S/N

51V

H2 16,000 30 1 51,000 39 0

He + H2 19,000 21 3 48,000 148 0

52Cr

H2 16,000 29 5 86,000 5.1 5

He + H2 26,000 0.83 14 130,000 6.8 20

55Mn

H2 82,000 0.13 250 180,000 0.47 300

He + H2 52,000 1.1 230 190,000 0.38 780

56Fe

H2 61,000 14 35 170,000 1.0 150

He + H2 46,000 5.2 20 170,000 11 50

57Fe

H2 64,000 57 2 180,000 11 9

He + H2 45,000 95 2 180,000 11 9

58Ni

H2 8,200 0.83 20 51,000 0.15 720

He + H2 14,000 2.2 40 70,000 1.9 465

59Co

H2 25,000 0.46 870 78,000 0.079 3700

He + H2 27,000 1.1 1100 100,000 0.27 460

63Cu

H2 3,600 16 50 27,000 4.4 150

He + H2 14,000 0.28 30 71,000 15 135

66Zn

H2 36,000 63 50 54,000 0.78 550

He + H2 30,000 57 50 54,000 18 120

75As

H2 1,700 5.8 80 1,600 3.4 50

He + H2 2,900 4.8 55 1,600 8.5 34

78Se

H2 6,700 39 30 2,800 46 30

He + H2 6,300 27 30 4,000 43 30

80Se

H2 6,900 60 4 2,800 49 3

He + H2 6,700 31 3 4,000 30 3

111Cd

H2 133,000 0.088 1600 66,000 1.1 510

He + H2 110,000 0.82 1700 61,000 1.5 285

208Pb

H2 270,000 0.49 500 84,000 0.47 1100

He + H2 250,000 0.80 600 110,000 1.8 690

16

interest (51

V, 52

Cr, 55

Mn, 56

Fe, 57

Fe, 58

Ni, 59

Co, 63

Cu, 66

Zn, 75

As, 78

Se, 80

Se, 111

Cd, and 208

Pb). The

reported sensitivity is corrected for percent abundance per isotope to demonstrate the total cps

for each element, allowing a more accurate comparison of sensitivities between elements and

isotopes. For example, using this scheme of reporting the two isotope pairs of Fe and Se, 56

Fe &

57Fe and

78Se &

80Se have identical sensitivities, within instrumental uncertainty, despite the

major difference in their respective isotopic abundance. In addition, Table 5.B. compares the best

detection limits achieved in the present study with the lowest concentrations (Bruland, 1983;

Donat & Bruland, 1995) from an expected seawater sample that has been pre-concentrated by a

factor of 20 (Milne et al, 2010). The detection limits range from 3 to 3,000 times lower than the

expected concentrations from the pre-concentrated seawater extractions.

The variability in analyte sensitivity in different acid matrices is due to the difference in

viscosities of the sample matrix that affects the sample uptake rate. In addition, elements with

low IP-1 and lighter mass (m < 65 amu) have a higher sensitivity and signal-to-noise ratio in cool

plasma mode versus the heavier elements (m > 65 amu) (Table 5). Based on this observation and

depending on the elemental isotope(s) of interest, the CRC operational mode (RM versus CRM)

was decided. For Fe, use of RM is preferred for 56

Fe as it efficiently eliminates 40

Ar16

O+ and thus

provides the best S/N. However, 57

Fe measurements are optimal with use of CRM as H2 reacts

with 40

Ar16

O+ and

56Fe

+ to create

40Ar

16O

1H

+ and

56Fe

1H

+, respectively, which both interfere with

57Fe. Operation of the CRC in CRM (H2 and He) instead of RM (H2) reduces the total amount of

H2 in the cell and thus minimizes reactions that lead to formation of H2 based polyatomics within

the CRC. Moreover, in CRM, the 40

Ar16

O1H

+ and

56Fe

1H

+ molecules upon formation are

removed through collision with He, thus resulting in a better S/N for 57

Fe (Table 5).

3.2 Plasma-based Interferences

Every isotope of Fe has a plasma-based Ar-polyatomic interference, making it a

challenging element for ICP-MS analyses. Figure 5 compares the limit of detection, blanks, and

air blanks between hot and cool plasma conditions for 56

Fe with and without the CRC in

operation (RM). With the CRC turned off (H2 = 0.0 mL/min), the hot plasma (1500 W)

conditions have a larger matrix blank and limit of detection than the cool plasma (600 W)

conditions. Argon has a very high first ionization potential (15.76 eV, versus Fe IP-1 = 7.87 eV),

therefore Ar is not as efficiently ionized in the weaker cool plasma compared to hot plasma.

Thus, there are fewer Ar based polyatomics in cool plasma with the CRC in RM (H2 = 4.7

17

mL/min), resulting in the 0.44 M HNO3 blanks being ~40% lower than in hot plasma (Figure 5).

With the Ar-based polyatomic interferences drastically reduced in cool plasma, accurate

determination of trace Fe in natural samples can be readily accomplished. For example, surface

seawater ([Fe]SW ≤ 2.7 x 10-12

mol/L) is concentrated by only a factor of 12-20 via a cation

chelating column in 1 mL of 1.0 M HNO3 (Milne et al, 2010).

Figure 5. Comparison of air blank, matrix blank (0.44 M HNO3) and limit of detection (LoD:

3σ) of Fe in hot and cool plasma mode (red and blue bars, respectively), with and without CRC

operation in RM. Checkered bars represent the LoD (cps), solid bars: matrix blank (cps), and

slashed bars: air blank (dry plasma). The gray region denotes the utilization of the CRC in RM.

In both plasma conditions, the blanks are reduced by ≥3 orders of magnitude in RM. Cool

plasma in RM achieves the lowest matrix blanks and best limit of detection due to fewer Ar-

based polyatomics forming in the plasma. Argon is not as efficiently ionized under cool plasma

(600 W) conditions compared to hot plasma (1500 W) due to its high IP-1 (15.76 eV).

Figure 6A shows the comparison between matrix blanks and sensitivity (per µg/L) for

56Fe under all operating conditions: hot plasma in CRM, hot plasma in RM, cool plasma in

CRM, and cool plasma in RM. In addition, the comparison includes the different acid matrices of

interest: 0.44 M HNO3, 1.0 M HNO3, and mixed acid (0.048 M HNO3 + 0.045 M HCl). In cool

plasma mode, the matrix blanks are generally lower for all acid matrices, especially with use of

RM (Figure 6A). Moreover, the Fe sensitivity is always high in cool plasma, regardless of which

18

Octopole CRC mode is adopted. The weaker cool plasma not only reduces the formation and

ionization of Ar interferent molecules, it also reduces the ionization efficiency of other elements

with high IP-1. This preferential ionization of low IP-1elements is due to the inefficient

ionization of high IP-1 elements (particularly Ar) diminishing the space charge effect in cool

plasma (Misra & Froelich, 2009), resulting in increased sensitivity for low atomic weight

elements (m/z ~<65). Based on the comparative evaluation of S/N, we conclude that the optimal

operating conditions for 56

Fe (and other elements of low atomic mass) analysis measurements in

any acid matrix involves the use of cool plasma with the CRC in RM mode (Figure 6B). While

the exact S/N values vary across acid matrices, the trend remains the same. To further highlight

the sensitivity comparisons for hot and cool plasma conditions for Fe, standard calibrations of

56Fe and

57Fe (Figure 7) demonstrate that sensitivity increases by a factor of ~3 over hot plasma

when cool plasma conditions are used. In addition, experiments were performed for 75

As, 78

Se,

and 111

Cd (Figure 6C – 6H). Unlike 56

Fe, these isotopes exhibit optimal S/N ratios under hot

plasma conditions in CRM.

Figure 6. Comparison of sensitivities (cps/1 µg·L-1

) and matrix blanks (cps) for 56

Fe (6.A), 75

As

(6.C), 78

Se (6.E), and 111

Cd (6.G) in all operating conditions: hot and cool plasma, Reaction

Mode (RM, H2 = 4.7 mL/min) and Collision-and-Reaction Mode (CRM, He = 2.8 mL/min and

H2 = 2.0 mL/min). The black bars denote 0.44 M HNO3 matrix blank, gray bars: 1.0 M HNO3,

and light gray bars: mixed acid (0.048 M HNO3 + 0.045 M HCl)). The ratio of the sensitivities

and matrix blanks can be represented as signal-to-noise ratios (S/N) (6.B, 6.D, 6.F, 6.H). 56

Fe

achieves the best S/N under cool plasma conditions with RM. However, 75

As, 78

Se, and 111

Cd all

generally exhibited optimal S/N ratios under hot plasma with CRM. These heavy isotopes (> 65

amu) are generally not as efficiently ionized in cool plasma as compared to 56

Fe.

19

20

Figure 7. Standard calibration in 0.44 M HNO3 of

56Fe (circles with solid lines, y1-axis) and

57Fe

(squares with dashed lines, y2-axis) operated under hot plasma (red) and cool plasma (blue)

conditions with the CRC in RM (H2 = 4.7 mL/min). Both 56

Fe and 57

Fe slopes increase by a

factor of ~3 when cool plasma conditions are applied. There is insignificant deviation from the

slope, including data in the low-concentration end of the calibration shown in the dark gray inset.

3.3 Matrix-based Interferences

Choice of sample matrix and its purity dictates both the type and magnitude of matrix-

based interference formation. For the present study, elements with major matrix-based

interferences include, but are not limited to, 51

V (35

Cl16

O+),

75As (

40Ar

35Cl

+),

111Cd (

95Mo

16O

+),

and 156

Eu (140

Ce16

O+). The

95Mo

16O

+ (m/z = 111) interference on

111Cd is caused by the presence

of 95

Mo in the analyte matrix. The relative abundance of Cd and Mo in the sample of interest

dictates the severity of this oxide-based interference. For seawater samples, [Cd]sw << [Mo]sw

([Cd]SW ≤ 4 x 10-10

mol/kg; [Mo]SW = ≤ 110 x 10-3

mol/kg (Milne et al, 2010; Boyle et al,

2012)), which makes accurate determination of Cd in seawater an analytical challenge.

Therefore, Cd is used as one of the examples in this study to demonstrate how matrix-based

interferences are overcome using the CRC. Similarly, 75

As has a large 40

Ar35

Cl+ (m/z = 75) based

interference for matrices containing Cl (e.g., halites, seawater, or presence of HCl in acid

matrix). The extremely small mass difference between 75

As+ (m/z = 74.9216) and

40Ar

35Cl

+ (m/z

= 74.9312) requires high resolution (M/ΔM = 10,000) mass spectrometry to achieve quantitative

21

peak separation between the two ions. However, inefficient ionization of As in the plasma (high

IP-1 – 9.81 eV) coupled with usually low abundance in natural samples makes determination of

As by HR-ICP-MS a serious analytical challenge. The application of Octopole CRC quasi-

quantitatively eliminates the polyatomic interference caused by 95

Mo16

O+

and 40

Ar35

Cl+,

rendering accurate and precise analysis of 111

Cd+ and

75As

+ possible without significant loss in

sensitivity (Figure 8).

Figure 8. 75

As standard calibration in mixed acid (0.048 M HNO3 + 0.045 M HCl) operated

under hot plasma (red) and cool plasma (blue) conditions, with RM (H2 = 4.7 mL/min, circles

solid lines) and CRM (He = 2.8 mL/min and H2 = 2.0 mL/min, squares with dashed lines)

employed. Hot plasma with CRM achieves sensitivity that is greater than the other operating

conditions by nearly a factor of ~2. There is insignificant deviation from the slope, including

data in the low-concentration end of the calibration shown in the dark gray inset.

Using single element Mo standards at different concentrations, we performed a series of

95Mo calibrations under all instrumental conditions: hot plasma and cool plasma, with CRM and

RM (Figure 9). Under the different plasma & CRC modes and across the Mo concentration range

of 0.1 µg/L to 2.0 µg/L, the intensity on 111 amu (95

Mo16

O) never exceeded 8 ng/L, which is

comparable to the detection limit of 111

Cd (≤3 ng/L, Table 5A). The formation of 95

Mo16

O+ does

not increase with the concentration of Mo in solution. This lack of mass dependency of the

22

95Mo

16O

+ interference on

111Cd demonstrates the successful removal of matrix-based polyatomic

interferences by Octopole CRC. The maximum instrumental sensitivity for both Cd and Mo are

achieved in hot plasma conditions using CRM (Figure 9 and 10). However, the next best

sensitivity for both elements is achieved in cool plasma with CRM, indicating that the Octopole

CRC setting dictates the sensitivity on Mo and Cd more than the plasma settings (Figure 9 and

10). For Cd analyses, the advantage of CRM over RM is that excess H2 is minimized in CRM.

This reduces the loss of analyte sensitivity that can result from reactions between Mo (or Cd) and

H2.

Figure 9. 95

Mo standard calibration (circles) in 0.44 M HNO3 executed in hot plasma with CRM

(He = 3.0 mL/min and H2 = 2.0 mL/min), hot plasma with RM (H2 = 4.7 mL/min), cool plasma

with CRM (He = 2.8 mL/min and H2 = 2.0 mL/min), and cool plasma with RM (H2 =4.8

mL/min). Measurements of 111 amu (squares) show complete elimination of 95

Mo16

O+ by the

Octopole CRC. The intensity on 111 amu never exceeds 8 ng/L, which is comparable to the

detection limit of 111

Cd (≤3 ng/L, Table 4A). The best sensitivities on 95

Mo is achieved from hot

and cool plasma with CRM while both cool settings in RM achieve very poor sensitivities,

suggesting that the CRC operational mode dominates the sensitivity on Cd more than the plasma

setting.

23

Figure 10. Comparison of sensitivity calibrations (slopes, cps/µg·L-1

) from a 111

Cd standard in

0.44 M HNO3, operated in hot and cool plasma (red and blue bars, respectively) with the CRC in

CRM and RM (white and gray regions, respectively). The solid bars represent the pure Cd

calibrations and the shaded bars are the Cd standards spiked with 1 µg/L Mo. Hot plasma with

CRM achieves maximum sensitivity and complete elimination of the 95

Mo16

O+

interference,

which is inferred from the identical slopes between the pure and spiked calibration. Cool plasma

with CRM also achieves complete elimination of the polyatomic interference, within (~2.0%).

However, hot and cool plasma with RM show greater variability (~3% and ~5%, respectively),

which supports the conclusion that the CRM has a greater affect on Mo (and Cd) than the plasma

setting.

To further investigate the efficiency of the CRC to remove the matrix-based 95

Mo16

O+

interferent on mass 111 and thus its effect on 111

Cd determination, the sensitivity calibrations

(slopes) of pure Cd standard solutions (0.1 – 2.0 µg/L) are compared to that of Cd standards

doped with 1 µg/L Mo. This comparison was performed for different plasma and CRC settings

(Figure 10). For the hot and cool plasma modes and RM and CRM settings, the average

difference in Cd sensitivity for pure Cd standards and Cd doped with Mo standards (≤ 2.0 %) is

within the instrumental uncertainty of Cd determination (< 1.5 %). The similarity in Cd

sensitivity of the two solutions demonstrates efficient elimination of 95

Mo16

O+ interference from

111Cd

+. Similar to Mo, ICP-MS operation under hot plasma with CRM results in best Cd

sensitivity, however cool plasma with CRM does not demonstrate similar efficiency for Cd

because Cd IP-1 (9.0 eV) is somewhat higher than Mo IP-1 (7.1 eV). Moreover, under both hot

24

and cool plasma conditions, greater Cd S/N is achieved in CRM over RM (Figure 10),

demonstrating that choice of the CRC operational mode is more important than selection of

plasma conditions.

3.4 Long-term Reproducibility

To assess the long-term reproducibility of the ICP-MS methods described in this work, an

external Standard Reference Material (NIST 1643e SRM) was analyzed over a period of 7

months (Figure 10) under all operational conditions and acid matrices. The NIST 1643e analyses

were performed at a 1:100 dilution of the original solution ([Fe] ≈ 1 µg/L and [Cd] ≈ 0.07 µ/L) to

match the analyte concentrations in actual samples. The results from the present study ([Fe]Average

= 99.6 ± 7.8 µg/L and [Cd]Average = 6.78 ± 0.83 µg/L; n = 26, ±2σ) are identical, within analytical

uncertainty of the instrument, to the certified values ([Fe]NIST-SRM = 98.1 ± 1.4 µg/L and [Cd]NIST-

SRM = 6.57 ± 0.07 µg/L) (Table 6).

Figure 11. SRM NIST 1643e (Standard Reference Material - trace elements in freshwater) Fe

and Cd concentration data collected over a period of 7 months. The SRM was analyzed at a

1:100 dilution in three different acid matrices (0.44 M HNO3, 1.0 M HNO3, or mixed acid (0.048

M HNO3 + 0.045 M HCl), which is not specified in this graph. Data was obtained under all

instrumental settings: hot plasma (red) and cool plasma (blue), with the CRC in RM (closed

symbols) and CRM (open symbols). The measured averages (black symbols, 2σ error bars) are

compared to the certified NIST 1643e values (green symbols, 2σ error bars).

25

Table 6. SRM NIST 1643e (Standard Reference Material- trace elements in freshwater) Fe and Cd concentration data collected over a period of 7

months (Figure 11). The SRM was analyzed at a 1:100 dilution in three different acid matrices (0.44 M HN03, 1.0 M HN0 3, or mixed acid (0.048 M

HN03 + 0.045 M HCl). The reported data includes operation of the Q-ICP-MS under four different instrumental settings: hot plasma and cool

plasma, and CRC operation in RM and CRM.

Date

J\llle 7th

J\llle 9th

J\llle 13th

J\llle 14th

July 1st

July 19th

July 20th

Sept. 9th

Oct. 14th

Oct. 16th

Oct. 17th

Dec. 15th

Dec. 16th

Dec. 18th

Jan. 16th

Average

Certified Value

Plasma CRC Mode Mode

Cool RM

Acid Matrix

1.0 M HN03

Mixed Acid

[Mg] ± 2cr [Fe] ± 2cr [Co]± 2cr [Ni] ± 2cr [As]± 2cr [Se] ± 2cr [Cd] ± 2cr [Sb] ± 2cr [Pb] ± 2cr

HセMエァ O lI@ HセMエァ O lI@ H セMエァ O l I@ H セMエ ァ O l I@ H セMエ ァ O l I@ HセMエァ O l I@ HセMエァOlI@ HセMエァ O l I@ HセMエァOlI@

8217

8018

n.a.

n.a.

n .a. n.a.

n.a. n.a.

Cool rRM 0.44 M HN0 3 8222

100.3

91.62

99.34

95.98

93.40

101.0

96.87

91.1 6

95.28

100.3

26.37

25.82

28.14

25.43

27.55

26.53

26.01

26.02

26.06

29.21

61.43

61.4 1

64.54

56.45

62.68

62.36

62.78

57.84

56.87

65.14

n.a.

11.18

13.00

12.36

8.52

10.28

12.06

8.22

10.26

13.42

8.54

6.57

6.27

7.21

5.91

7.00

6.54

6.59

6.13

6.37

7. 12

n.a. n.a.

Hot

Hot

Cool

Hot

Hot

Hot

Hot

Hot

Hot

Hot

Hot

Cool

Cool

1.0 M HN03 8768 n.a. n.a. n.a.

Mixed Acid 8343 n.a. n.a. n.a.

RM 0.44 M HN03 7800 n.a. n.a. n.a.

1.0 M HN03 8368 n.a. n.a. n.a.

Mixed Acid 7970 n.a. n.a. n.a.

CRM 0.44 M HN03 8 179 n.a. n .a. n.a.

RM

RM

RM

RM

RM

RM

RM

CRM

RM

RM

CRM

Mixed Acid 9180

1.0 M HN03 8179

0.44 M HN03 7892 ± 45.8

0.44 M HN03 7925 ± 266

0.44 M HN03 8270 ± 302

0.44 M HN03 7865 ± 50.6

0.44 M HN03 7977 ± 857

0.44 M HN03 7825 ± 463

Mixed Acid 8208

0.44 M HN03 8794

Mixed Acid 8040

Mixed Acid 7 439

96.72 26.28

103.0 ± 3.10 28.26 ± 0.68

104.7 ± 0.79 28.88 ± 1.0 I

102.1 ± 6.79 27.43 ± 1.55

101.2 ± 4.60 27.35 ± 0.1 6

102.1 ± 0.73 27.00 ± 0.40

101.0 ± 0.25 27.33 ± 0.31

99.93 28.09

104.8

95.97

98.97

27.52

26.30

25.02

n.a.

58.05 n.a.

63.81 n.a.

64.09 ± 0.18 54.33 ± 0.21

63.10 ± 0.26 52.85 ± 1.33

64.1 4 ± 5.65 58.34 ± 6.26

62.47±0.18 55.36 ± 4.10

62.83 ± 3.32 58.69 ± 0.04

64.08 58.93

66.27

60.93

57.13

54.79

n.a.

n.a.

9.92 6.21

13.90 ± 0.87 6.82 ± 0.22

13.63 ± 0.52 6.88 ± 0.26

12.63 ± 0.77 6.63 ± 0.26

n.a. 7.13 ± 0.04

n.a. 7.24 ± 0.44

n.a. 7.37 ± 0.70

n.a. 6.73

n.a.

n.a.

n.a.

6.37

6.77

7.24

n .a.

n .a.

n .a.

56.76 ± 6.03

58.56 ± 3.31

60.94 ± 0.18

60.46 ± 0.26

61.33 ± 0.05

60.91

59.25

59.30

53.83

n.a.

n.a.

n.a.

19.72 ± 0.52

20.44 ± 0.51

19.68 ± 0.52

19.71 ± 0.12

20.00 ± 0.59

19.83

19.61

20 02

20 .1 2

8 166 ± 773 99.60 ± 7.80 26.98 ± 2.27 61.83 ± 5.82 56.18 ± 4.87 11.28 ± 4.00 6.78 ± 0.83 59.04 ± 4.85 19.90 ± 0.53

8037 ± 83.3 98.10 ± 1.40 27.06 ± 0.28 62.4 1 ± 0.65 60.45 ± 0.63 11 .97 ± 0.12 6.57 ± 0.07 58.30 ± 0.60 19.63 ± 0.20

n

I

2

2

2

2

2

2

I

26

CHAPTER 4

CONCLUSIONS

We present an improved method for accurate and precise determination of trace metals in

natural samples via utilization of an Octopole Collision – Reaction Cell equipped Agilent®

7500cs Quadrupole-ICP-MS. This method focuses on elements with plasma- and/or matrix-

based mass interferences for ICP-MS analysis, such as 56

Fe, 75

As, 78

Se and 111

Cd. The present

method can be applied to samples in matrices with different composition (with or without HCl)

to measure multiple elements in a single analysis across a large dynamic concentration range.

Using the methods described in this study, the relatively low cost for Q-ICP-MS/CRC

instrumentation offers new analytical possibilities in chemical oceanography, environmental

geochemistry, forensic science, and many other fields where difficult sample matrices are

encountered.

27

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30

BIOGRAPHICAL SKETCH

EDUCATION:

May 2013 M. Sc. in Chemical Oceanography

Florida State University, Tallahassee, FL

May 2010 B. Sc. in Chemistry

Florida State University, Tallahassee, FL

PRESENTATIONS:

Dial A., Ridgewell C., Kilgore B., Tremaine D.M., Misra, S. & Salters V.J.M. (2012).

Improved analytical method for determination of Mg isotopes: Application to seawater

and natural carbonates. V.M. Goldschmidt, Montreal, QC, Canada; Published in

Mineralogical Magazine, 76 (6), 1650 (2012).

POSTERS:

• Dial A., Misra S., Landing W. M. (2011). Accurate and precise determination of iron

concentrations by ORC equipped Quadrupole-ICP-MS: Application to low concentration

natural samples. ACS, FAME 2011, Palm Harbor, FL.

• Dial A., Misra S., Landing W. M. (2011). Accurate and precise determination of iron

concentrations by ORC equipped Quadrupole-ICP-MS: Application to low concentration

natural samples. Gordon Research Conference 2011, Andover, NH.

PROFESSIONAL MEMBERSHIP:

Geochemical Society