PMP – Particle Measurement Program UNECE Informal Group Non-exhaust particle emissions Working Item 4 Development of a set of recommended measurement techniques and sampling procedures Questions related to the present document Q1. Is the content of the document appropriate? Does it cover the main aspects discussed during the last face-to-face meeting? Q2. Is the template sufficient and easy to process? Do the tables cover the most important aspects regarding methodologies? Q3. Is there any additional information that needs to be added? Please provide comments/suggestion This document provides an overview of the main generation/sampling/measurement techniques/methodologies described in publicly available studies and used to investigate particle emissions from brake and tyre wear. All references used in this document can be found in the survey of the available literature conducted by the JRC. This document is intended to provide a basis for further discussion for the development of a set of recommended methodologies and techniques with the final objective of improving the comparability of future studies and their outcomes. 1. Generation and sampling of wear particles 1a. Brake wear particles Brake wear particles generation and sampling can be performed in the laboratory by means of a roller chassis bench (Full Chassis Dynamometer), a brake dynamometer or a pin-on-disc configuration. Furthermore, mobile units can be employed in order to sample brake wear particles on-road under “real world” driving conditions. Table 1 gives an overview of the methods used for brake wear particles generation and sampling. Table 1: Overview of methods used for brake wear particles generation and sampling Code Method Note Open System G1 Brake Dynamometer Enclosed System G2 G3 G4 G5 G6 G7 Pin-on-disc method Roller Bench (Full Chassis Dynamometer) Mobile Unit Open System Enclosed System Open System Enclosed System Open System References Iijima et al. 2007 Österle et al. 2008 Österle et al. 2010 Sanders et al. 2003 Garg et al. 2000 Gasser et al. 2009 Iijima et al. 2008 Kukutschová et al. 2009 Kukutschová et al. 2011 Mosleh et al. 2004 Wahlstrom et al. 2010a Wahlstrom et al. 2010b Kwak et al. 2013 Mathissen et al. 2011 Figure 1a provides a schematic representation of two different brake dynamometer assemblies (Iijima et al. 2007; Kukutschová et al. 2011). The most important difference among the two assemblies is that the second one is enclosed in an environmental chamber. In Figure 1b an enclosed pin-on-disc assembly is depicted (Wahlstrom et al. 2010b). Close systems have several advantages over open ones. One advantage is the knowledge that the particles collected and measured originate from the wear of the brake assembly and not from the surroundings. The background concentration could be in the same order or higher than the concentration produced by the disc brake contact, especially if urban driving conditions are studied. This also means that resuspension of existing particles is ruled out, thus no under- or over- estimation of wear particles due to resuspension occurs. With close systems is easy to provide the right conditions for isokinetic sampling and a high particles collection efficiency, as industrial benches have big safety chambers where proper piping systems can be installed. Another advantage of close over open systems is that it is possible to control the cleanness of the incoming air. Furthermore it is possible to precisely control the temperature and humidity levels. On the other hand, determined particle size distribution in open systems cannot deviate from the original due to particle aggregation or deposition as a result of the interaction between the particles and the chamber wall. It is true that the real brake system does not work in a completely free environment either, because on one side there is the rim and on the other side the mudguard, therefore the influence of the close chamber (or the lack of it) cannot be evaluated. Figure 1a: Schematic representation of different brake dynamometer assemblies [Left Iijima et al. 2007; Right - Kukutschová et al. 2011] Regarding mobile units, Mathissen et al. 2011 equipped a vehicle with five stainless steel sampling tubes of 0.4 cm in diameter inside the front right wheel housing. The different positions allow the localization of the particle source. Conductive tubing with an inner diameter of 0.8 cm and an average length of 6 m was used to connect the sampling ports with the measurement devices inside the vehicle. The setup is not designed for isokinetic sampling. However, there is no correction necessary since non-isokinetic sampling losses would have affected larger particles only. The residence time for the aerosol can be estimated to be smaller than 0.4 s at a flow rate of 50 l min-1. Thermophoresis can be neglected because the measurements were performed at ambient temperature. On the other hand, Kwak et al. 2013 equipped a vehicle with three sampling inlets, one in front of the vehicle to measure background concentrations, one close to the tire/road interface to measure tyre particles, and one close to the brake pad to sample brake particles. All sampling inlets were connected to sampling plena, which had an inner diameter of 48 mm, enabling the sampling air-flow to be well mixed. Flow velocity of sampling air was 0.58 m/s, and the Reynold's number was 1858, thus satisfying laminar flow. Sampling particles were sucked in at a flow rate of 63 l min−1. Conductive tubing with an inner diameter of 10 mm and length of 1 m was to line the tubes running from the plena to the particle monitors. Isokinetic sampling design was adopted. Figure 1b: Schematic representation of a pin-on-disc assembly. (A) Room air; (B) fan; (C) flow rate measurement; (D) filter; (E) flexible tube; (F) inlet for clean air, measurement point; (G) closed chamber; (H) pin-on-disc machine; (I) pin sample; (J) air outlet, measurement points; (K) displacement gauge; (L) dead weight; (M) rotating disc sample; (N) air inside chamber, well mixed [Wahlstrom et al. 2010b] 1b. Tyre wear particles Tyre wear particles generation and sampling can be performed either by directly in the laboratory using a wheel simulator or on-road, under “real world” driving conditions, by means of mobile units. In general, road simulation laboratory studies are employed in order to study the contributions from tyre and road wear in an isolated environment, under controlled laboratory conditions, whereas the mobile units usually measure additionally the contribution from resuspended dust present under ambient conditions. Finally, cryogenic production of tyre wear particles can be performed if pieces of tread are crushed under cryogenic conditions and sieved to 180 μm. However, this methodology generates only very large particles and fails to represent actual wear conditions. Figure 2 provides a schematic representation of three different road simulators (Gustafsson et al. 2008; Aatmeeyata et al. 2010; Kreider et al. 2010). Details on all simulators are provided in the annex. The set-up depicted on the left was used in Aatmeeyata et al. 2010 and is designed to utilize vertical space and thus reduce space requirement and enable complete enclosure of the entire set-up (1.8 x 0.71 x 1.28 m). The fork/wheel assembly is also equipped with a brake, while an odometer is used to measure the speed of rotation and (linear) distance traveled by the tire. At the top of the assembly, there is a provision for applying a load on the tire. On the other hand, sampling in the VTI simulator hall makes it possible to sample pure wear particles, with very low contamination from ambient particles and no influence from tail-pipe emissions. The VTI road simulator is possible to run with four wheels around a circular track. A linear track simulation is accomplished even though the tires are running in a circle, because no radial force is acting on the tires as the wheels are bolted to the axles of the road simulator. To make the wheels move radically across the entire track, an eccentric movement can be activated above 50 km h-1. The simulator track can be equipped with any type of pavement. The dimensions of the simulator are 10 m x 8 m x 5 m. Lastly the Bundesanstalt für Straßenwesen (BASt), the German Federal Highway Research Institute, operates an interior drum testing system (IPS) that consists of an enclosed drum that contains pavement casks against which a tire can roll. The IPS has an internal diameter of 3.8 m and is electronically programmable to mimic a variety of driving conditions by varying speed, temperature, acceleration, braking, and steering. Tire wear particles are generated without the influence from other road surface contaminants such as brake dust, vehicle exhaust, oil/grease, salts, soil, vegetation, etc. For both the VTI and BASt road simulators, the pavement is not subjected to weathering or other natural conditions, and as such a polishing effect can occur that causes the surface becomes smoother. Therefore, the pavement is ‘sharpened’ between runs to maintain representative surface textures. Table 2: Overview of methods used for tyre wear particles generation and sampling Code Method G8 Road - Wheel Simulator G11 Open System Enclosed System G9 G10 Note References Dahl et al. 2006 Gustafsson et al. 2008 Kupiainen et al. 2005 Panko et al. 2009 Sjodin et al. 2010 Aatmeeyata et al. 2009 Aatmeeyata et al. 2010 Kreider et al. 2010 Kreider et al. 2010 Rogge et al. 1993 Cryogenic Production Mobile Unit Open System Hussein et al. 2008 Kreider et al. 2012 Kwak et al. 2014 Mathissen et al. 2011 Figure 2: wheel simulators used in different studies [Up-left: Aatmeeyata et al. 2010; Upright: Gustafsson et al. 2008; Below: Kreider et al. 2010] Regarding mobile units, those developed by Mathissen et al. 2011 and Kwak et al. 2013 were described in 1a section. Hussein et al. 2008 equipped a vehicle with three metal tube inlets: two behind the front tires and one underneath the van as a background. The front inlet was 0.4 cm in diameter and 3 m long; the flow rate in this inlet was 1.7 l m-1. Both inlets behind the front tires were mounted symmetrically and they were 1.9 cm in diameter and 2.3 m long. Flow rates through these two inlets were 75 l m-1. Measurements behind the tires during motion indicated that along the center of the tire, the air speed is not significantly influenced by the ambient wind direction at distances of 10 cm from the tire. Each inlet behind the left and right tires fed into a 60-cm-long torpedo-shaped manifold that had an inner diameter of 7.5 cm. A specially designed baffle ensured that the flow through the manifold was uniform and well mixed. A single carbon vane pump drew the necessary air through both the manifolds. The manifold was used to distribute the sampled air to as many as five instruments which were connected to the manifold via 100-cm-long tygon tubes. 2. Physicochemical characterization of wear particles 2a. Mass Size distribution measurement systems The most commonly used instruments for assessing mass weighted size distribution are cascade impactors, which operate on the basis of inertial classification of particles. Even if different kinds of impactors have been employed for assessing wear particles, they all operate based on the same principal. Another commonly used method for assessing mass weighted size distribution involves the use of an Optical Particle Counter. Table 3 gives an overview of the methods used in the literature. More details for each method can be found in the Annex. Table 3: Overview of methods used for mass size distribution of wear particles Code M1 M2 M3 M4 Instrument Principle Optical Particle Counter (DustTrak) Light scattering with electrical detection Wahlstrom et al. 2010a Wahlstrom et al. 2010b Inertia impaction Harrison et al. 2012 Micro Orifice Uniform Deposit Impactor (MOUDI) Small deposit area low-pressure cascade impactor (SDI) Low Pressure Impactor (LPI) Brakes Garg et al. 2000 Gietl et al. 2010 Harrison et al. 2012 Sanders et al. 2003 Inertia impaction Inertia impaction Tyres Gustafsson et al. 2008 Hussein et al.2008 Kreider et al. 2012 Kwak et al. 2013 Panko et al. 2009 Sjödin et al. 2010 Gustafsson et al. 2008 Kupiainen et al. 2005 Panko et al. 2009 Sjödin et al. 2010 Kukutschová et al. 2011 Österle et al. 2008 Österle et al. 2010 2b. Number Size distribution measurement systems Particle size measurement can be based on the following properties: geometrical size (Microscopy), inertia (Impactors), electrical mobility (Differential Mobility Analysers), and optical properties (Optical Particle Counters). These properties have been used by researchers for assessing PN distribution of wear particles. Table 4 gives an overview of the methods used in the literature. More details for each method can be found in the Annex. Table 4: Overview of methods used for number size distribution of wear particles Code N1 Instrument Laser Scattering Particle Size Analyzer (LSA) N2 Aerodynamic Particle Sizer (APS) N3 Engine Exhaust Particle Sizer (EEPS) N4 Condensation Nucleus Counter (CPC) N5 Aerosol Spectrometer – Optical Particle Counter (OPC) N6 Scanning Mobility Particle Sizer (SMPS) N7 Electrical Low Pressure Impactor (ELPI) Principle Brakes Light scattering Kukutschová et al. 2009 Mosleh et al. 2004 Inertia impaction with light scattering detection Differential mobility analysis with electrical detection Condensation of particles with light scattering detection Light scattering with electrical detection Electrical mobility analysis with electrical detection Electrical impaction with electrical detection Iijima et al. 2007 Iijima et al. 2008 Kukutschová et al. 2011 Sanders et al. 2003 Tyres Gustafsson et al. 2008 Kreider and Panko, 2012 Kwak et al. 2013 Panko et al. 2009 Sjödin et al. 2010 Mathissen et al.2011 Österle et al. 2010 Wahlstrom et al. 2010a Wahlstrom et al. 2010b Österle et al. 2008 von Uexküll et al. 2005 Wahlstrom et al. 2010a Wahlstrom et al. 2010b Kukutschová et al. 2011 Österle et al. 2008 Wahlstrom et al. 2010b Aatmeeyata et al. 2009 Hussein et al.2008 Dahl et al. 2006 Gustafsson et al. 2008 Panko et al. 2009 Sjödin et al. 2010 Garg et al. 2000 Sanders et al. 2003 An important issue to be taken into account when studying particle size distributions is that in order to fully describe the distribution it is necessary to use instruments that cover the whole range of the particles’ size. For instance in case of PN distribution a combination of a SMPS and an optical counter would cover the whole range of diameters between a few nm to several μm. On the other hand, studies that use instruments with specific limitations at their measurement range may result in misleading conclusions like those previously recorded at the PMP group (i.e. APS or other optical counters with a detection limit of around 0.3 µm). Figure 3 depicts an idealized size distribution (upper line) in which SMPS measurements of ultrafine particles together with APS measurements (bottom separated lines) have been combined. Since APS has a detection limit of 300-400 nm it gives an artificial mode in this size fraction. The same occurs with SMPS alone for the coarser size fractions. To avoid these artefacts close to the edge of the coarser and finer detection limits, the size distributions have to be recalculated to give a continuous size distribution (upper one). Figure 3. Size distribution in which SMPS measurements of ultrafine particles together with APS measurements are combined (upper line) or separated (bottom lines) 2c. Chemical and morphology characterization Table 5 gives an overview of the methods used in the literature for the chemical and morphology characterization of particles emitted as a result of brake and tyre wear. Most of these methods refer to the chemical characterization of the inorganic part of wear particles (i.e. trace elements and heavy metals). Very few studies tried to identify specific organic compounds into wear particles and this remains a field where there is still a lack of information. Like in case of size number distribution, in order to fully characterize wear particles it is necessary to combine two or more analytical methods, since each one of them comes with specific limitations. More details for each method, as well as for the combinations found in the literature are given in the Annex. Table 5: Overview of methods used for chemical characterization of wear particles Code Instrument Principle Brakes C1 Scanning Electron Microscope (SEM) Electron interaction with visual detection C2 Transmission Electron Microscope (TEM) Electron interaction with visual detection C3 X-Ray Fluorescence (XRF) Detection of X-Ray fluorescence C4 C5 C6 C7 C8 C9 C10 C11 C12 Kukutschová et al. 2009 Kukutschová et al. 2011 Österle et al. 2008 Österle et al. 2010 Peikertová et al. 2013 Wahlstrom et al. 2010a Gasser et al. 2009 Kukutschová et al. 2011 Österle et al. 2008 Österle et al. 2010 Peikertová et al. 2013 Tyres Adachi et al. 2004 Camatini et al. 2001 Gustafsson et al. 2008 Kreider et al. 2010 Kupiainen et al. 2005 Panko et al. 2009 Sjödin et al. 2010 Kukutschová et al. 2011 Sanders et al. 2003 Harrison et al. 2012 Karlsson et al. 2011 Kukutschová et al. 2009 Mosleh et al. 2004 Österle et al. 2008 Österle et al. 2010 Wahlstrom et al. 2010a Adachi et al. 2004 Camatini et al. 2001 Gustafsson et al. 2008 Kupiainen et al. 2005 Panko et al. 2009 Sjödin et al. 2010 Energy Dispersive XRay Spectroscopy (EDX or EDS) Detection of XRay dispersive energy X-Ray Diffraction Spectroscopy (XRD) Proton Induced X-Ray Emission (PIXE) X-Ray diffraction patterns for detection Peikertová et al. 2013 von Uexküll et al. 2005 X-Ray detection Garg et al. 2000 Kukutschová et al. 2011 Gustafsson et al. 2008 Panko et al. 2009 Sjödin et al. 2010 Oxidation of PM with optical detection Conversion to plasma and atomic emission detection Garg et al. 2000 Kukutschová et al. 2011 Aatmeeyata et al. 2010 Kupiainen et al. 2005 Iijima et al. 2007 Iijima et al. 2008 Kreider et al. 2010 Conversion to plasma and m/z detection Iijima et al. 2007 Iijima et al. 2008 Sjodin et al. 2010 Rogge et al. 1993 Thermal/Optical Carbon Analyzer Inductively Coupled Plasma – Atomic Emission Spectroscopy (ICP-AES) Inductively Coupled Plasma – Mass Spectrometry (ICP-MS) Gas Chromatography Mass Spectrometry (GC-MS) Column separation and m/z detection High Pressure Liquid Chromatography Fluorescence Detector (HPLC-FLD) Pyrolysis with Gas Column separation and fluorescence detection Thermal Aatmeeyata et al. 2010 Kreider et al. 2010 Kwon et al. 2012 Rogge et al. 1993 Sjodin et al. 2010 Unice et al. 2012 Chromatography-Mass Spectrometry C13 Focused ion beam microscopy decomposition of PM with m/z detection Ion interaction with visual detection Milani et al. 2004 Annex A. Generation and sampling of wear particles Brake wear particles G1 Commercial name(s) Type of instrument Temperature tolerance Braking Pressure or Deceleration Speed variation Inertial load What can measure What cannot measure Main limitations Main Characteristics / Advantages G2 Commercial name(s) Type of instrument Temperature tolerance Braking Pressure or Deceleration Speed variation Inertial load What can measure What cannot measure Brake Dynamometer Link full-scale brake dynamometer (2900); TecSA Intertia Dynamometer Brake Dynamometer Up to 700-800°C Up to 4.9 m s-2 0–90 km/h 45-90 kg m2 Can be coupled to size distribution instruments; Filters can collect PM for characterization; Speed, Acceleration, Deceleration, Pressure, Torque, Brake temperature, cooling air speed, air temperature Live wear value. It has to be done by getting pin/disc dimensions before and after test; Not appropriate for investigation of generation mechanism Not possible to control the cleanness of the incoming air and or precisely control the temperature and RH levels; Not appropriate for investigation of generation mechanism; Difficulty of reproducing the conditions and loads identical as on real vehicle. Deviation from reality could come from: air and rolling resistance, real torque (instantaneous) distribution, air flow. Open System / High repeatability, accuracy and automation of the tests (no human factor affecting the test); Short time of execution; Able to reduce the particle collection efficiency and modify the dilution factor (especially from high energy brakes which emits a PN which can create instruments problems - overflow, unreliable currents) Brake Dynamometer Link Friction Test Machine (D); Link full-scale brake dynamometer (2900); TecSA Intertia Dynamometer Brake Dynamometer Up to 400°C Up to 4.9 m s-2 0–180 km/h 120-2000 kg Can be coupled to size distribution instruments; Filters can collect PM for characterization; Speed, Acceleration, Deceleration, Pressure, Torque, Brake temperature, cooling air speed, air temperature Live wear value. It has to be done by getting pin/disc dimensions before and after test; Not appropriate for Main limitations Main Characteristics / Advantages investigation of generation mechanism Particle size distribution may deviate (?) from the original due to particle aggregation or deposition as a result of the interaction between the particles and the chamber wall; Not appropriate for investigation of generation mechanism; Difficulty of reproducing the conditions and loads identical as on real vehicle. Deviation from reality could come from: air and rolling resistance, real torque (instantaneous) distribution, air flow. Close System / High repeatability, accuracy and automation of the tests (no human factor affecting the test, no ambient influence); Short time of execution; Can be a good mean to understand if pin-on-disc studies are somehow significative of a real system; Able to reduce the particle collection efficiency and modify the dilution factor (especially from high energy brakes which emits a PN which can create instruments problems - overflow, unreliable currents) G3 Pin-on-disc Tribometer Commercial name(s) Type of instrument Temperature tolerance Braking Pressure or Deceleration Speed variation Inertial load Not applicable Tribometer What can measure Up to 2-3 MPa depending on pin geometry 60 km/h Not applicable Can be coupled to size distribution instruments; Speed, Acceleration, Deceleration, Pressure, Brake temperature, air temperature, relative humidity What cannot measure Main limitations Main Characteristics / Advantages Not possible to reach speeds higher than those of urban conditions; Not possible to control the cleanness of the incoming air and or precisely control the temperature and RH levels; Possible contamination from resuspension dust Open System; Appropriate for investigation of generation mechanism; Can be used to determine wear and airborne wear coefficients which could be used in computer simulations G4 Pin-on-disc Tribometer Commercial name(s) Type of instrument Temperature tolerance Braking Pressure or Deceleration Speed variation Inertial load Not applicable Tribometer What can measure What cannot measure Up to 2-3 MPa depending on pin geometry 60 km/h Not applicable Can be coupled to size distribution instruments; Speed, Acceleration, Deceleration, Pressure, Applied torque, Brake temperature, Air temperature, Relative humidity Main limitations Main Characteristics / Advantages Not possible to reach speeds higher than those of urban conditions; PN distribution may deviate from the original due to particle aggregation or deposition as a result of the interaction between the particles and the chamber wall Close System; Appropriate for investigation of generation mechanism; Can be used to determine wear and airborne wear coefficients which could be used in computer simulations Tyre wear particles G8 Road - Wheel Simulator Commercial name(s) Type of instrument Temperature tolerance Acceleration or Deceleration Speed variation Inertial load VTI road simulator Road simulator Unlimited What can measure Up to 70 km/h Axle load 450 kg Can be coupled to size distribution instruments; Speed, Acceleration, Deceleration, air temperature, relative humidity What cannot measure Main Characteristics / Advantages Not possible to control the cleanness of the incoming air and or precisely control the temperature and RH levels Open System; Appropriate any type of pavement G9a Road - Wheel Simulator Commercial name(s) Type of instrument Temperature tolerance Acceleration or Deceleration Speed variation Inertial load Not applicable Wheel simulator Unlimited Main limitations What can measure 36 km/h 44.3 kg Can be coupled to size distribution instruments; Speed, Acceleration, Deceleration, air temperature, relative humidity What cannot measure Main limitations Main Characteristics / Advantages Not possible to achieve high speeds; PN distribution may deviate from the original due to particle aggregation or deposition as a result of the interaction between the particles and the chamber wall Close System; Reduced space requirement; Complete enclosure of the entire set-up that facilitates collection of all generated particles G9b Road - Wheel Simulator Commercial name(s) BASt road simulator Type of instrument Temperature tolerance Acceleration or Deceleration Speed variation Inertial load What can measure Road simulator -10°C to 50°C Acceleration: 0-63 m/s2; deceleration: 0.5 - >2 m/s2 Up to 160 km/h Maximum wheel load 10kN Can be coupled to size distribution instruments; speed, acceleration, deceleration, air temperature, tire temperature, camber angle, steering angle What cannot measure Main limitations Main Characteristics Complex ventilation system and airflows inside the drum make real-time particle size distribution difficult Closed System; Appropriate for any type of pavement; ability to set variable driving par cour; cyclonic collection device to collect bulk wear particulate can be mounted inside near tire pavement interface B. Mass Size distribution measurement systems M1) DustTrak aerosol monitor is a fast Optical Particle Counter (OPC) which measures the volume concentration and reports the mass concentration of particles in mg/m3. It is based on light scattering and can measure particle concentrations corresponding to the respirable size in the range of 0.001–150 mg/m3 with 1 s time resolution (Kwak et al. 2013). The instrument is calibrated with a standardized test dust having a different size distribution, density, and refractive index from those of the particles measured here. A disadvantage of OPCs is that uncertainty in refractive index often leads to significant variability in derived size distributions, even for the ideal case of homogeneous spherical aerosol particles. Although the output of the DustTrak OPC can only be used as a relative measure, it is useful for detecting changes over time in the generated particle mass (Wahlstrom et al. 2010a; Wahlstrom et al. 2010b). It is not approved for air quality surveillance against air quality guidelines but it is useful for monitoring of fast courses of events in homogenous aerosols (Sjodin et al. 2010). M2) Micro-Orifice Uniform Deposit Impactor (MOUDI) is a cascade impactor that separate particles according to their aerodynamic size. It operates on the basis of inertial classification of particles. The aerosol sample passes through a succession of stages, at each of which the aerosol is directed through an array of nozzles situated above a solid substrate. Particles with aerodynamic diameters above the design cut-point deposit by impaction, whereas smaller particles follow gas streamlines around the collection plate. Impaction efficiency is a function of Stokes number. The narrower the nozzle and the higher the air velocity, the finer are the particles that are collected. The smallest particles passing through the final stage cannot be collected due to their small inertia, but often are collected onto a final filter (Giechaskiel et al. 2014). MOUDI can be adjusted to operate with a different number of collection stages (from 5 to 11) with the D50% cut points ranging from 56 nm to 18 μm. Aluminium foils are used for the collection of the particles. Foils are weighed before and after collection of the wear debris to determine directly the mass-weighted size distribution. MOUDI mainly deals with the non-volatile material leading at an overall underestimation due to particle loss by vaporization (Harrison et al. 2011). Additionally, impactors in general are subject to errors due to particle bounce which tends to reduce the measured particle size (Garg et al. 2000). M3) Small deposit area low-pressure cascade impactor (SDI) is used to collect highly size-resolved aerosol particle samples in several size fractions (aerodynamic cut-off diameter between 0.045 and 8.39 μm), with a sample flow rate of 11 l/min. Like all impactors it operates on the basis of inertial classification of particles. The relatively high sample flow rate together with the small particle collection area (Ø 8 mm), increase the sensitivity of the particle analysis even when the sample concentration is low, while on the other hand low pressure makes this technique inappropriate for volatile particles. Nuclepore polycarbonate membrane filters are usually employed as collection substrates. M4) Low Pressure Impactor (LPI) is a multi-stage cascade low pressure impactor which is used to determine particle gravimetric mass size distribution. It operates on the basis of inertial classification of particles. The size classification in LPI is made from few nm up to 10 µm with evenly distributed impactor stages and can be extended down to 30 nm with an additional back-up filter. Aluminum foils coated with a polycarbonate film and a thin layer of vacuum grease are used as impaction substrates. In each size fraction the particles are collected on 25 mm collection substrates that are weighed before and after the measurement to obtain gravimetric size distribution of the particles. Other LPI characteristics include low inter-stage wall-losses and robust yet easy-to-use operation. C. Number Size distribution measurement systems N1) Laser Scattering particle size distribution Analyser (LSA) is used to measure particles with diameters from 20 nm up to 1000 μm. The principle is based on measuring the angular variation in intensity of light scattered as a laser beam passes through a dispersed particulate sample. Large particles scatter light at small angles relative to the laser beam and small particles scatter light at large angles. The angular scattering intensity data is then analysed to calculate the size of the particles responsible for creating the scattering pattern, using the Mie theory of light scattering. The shorter the wavelength of the irradiated light, the smaller the diameter becomes of particles that can be measured. The particle size is reported as a factor of volume, area, length or particle number (Kukutschová et al. 2009). N2) The Aerodynamic Particle Sizer (APS) provides real-time aerodynamic measurements of particles from 500 nm to 20 μm. The APS counts particles of all size fractions at each instant of the sampling period and allows for the monitoring of particle size distribution and size variation during the entire period of the test cycle. The particle size is calculated as the aerodynamic diameter from the time of flight for passing between two laser beams. Since the APS spectrometer has high signal response, it is possible to obtain the short-time profiles of particle size distribution (Iijima et al. 2007). APS measures the number concentration as a function of the aerodynamic particle diameter. Mass concentrations can also be calculated assuming a density of about 2,800 kg/m3 (Sjodin et al. 2010). N3) An Engine Exhaust Particle Sizer (EEPS) consist of a particle charger, a classification column, and a series of detectors and it is used for on-line measurement of particle size distributions in the range from 5.6 to 560 nm. The instrument draws a sample of the particle flow into the inlet continuously. Particles are positively charged to a predictable level using a corona charger. Charged particles are then introduced to the measurement region near the centre of a high-voltage electrode column and transported down the column surrounded by HEPA-filtered sheath air. A positive voltage is applied to the electrode and creates an electric field that repels the positively charged particles outward according to their electrical mobility. Charged particles strike the respective electrometers and transfer their charge. A particle with higher electrical mobility strikes an electrometer near the top; whereas, a particle with lower electrical mobility strikes an electrometer lower in the stack. This multiple-detector arrangement using highly sensitive electrometers allows for simultaneous concentration measurements of multiple particle sizes. The use of a corona discharge is necessary to compensate for the lower detection sensitivity of electrometers versus CPCs. The drawback is that the corona creates a significant fraction of multiply charged particles which are detected at commensurately lower size. Hence, inversion of the current distribution becomes a complex process. This explains the sometimes large differences between the results from these mobility spectrometers as compared to SMPS derived size distributions. These differences can translate as well to mass differences compared to filter or other mass based instruments. Mobility spectrometers have lower sensitivity and size resolution than the SMPS, but their high time resolution (0.1–1 Hz) is advantageous for transient measurement. N4) PTrak counter is a particle measurement instrument which use light scattering to count particles in real time after they are grown to micron size range between 0.02 and 1 μm. The P-trak ultrafine particle counter is a portable version of a condensation particle counter (CPC). The working principle of PTrak is more or less the same of all CPCs. Particles are drawn through the instrument by a pump. Upon entering the instrument, particles pass through a saturator tube where they mix with alcohol vapours. The particle/alcohol mixture is then drawn into a condenser tube, which cools the air/particle stream causing alcohol to condense on the particles and the particles grow into detectable droplets. The droplets then pass through a focused laser beam, producing flashes of scattered light. The scattered light flashes are sensed by photodetector and counted to determine particle number concentration. The temperatures of the saturator and condenser and properties of the working fluid determine the lower detectable size, which is typically in the range of 3–10 nm. The CPCs in the European legislation must be full-flow (the total inlet flow must pass the counting optics), and have a 50% counting efficiency at 23 nm. N5) Optical Particle Counters (i.e GRIMM 1.108 and 1.109) are aerosol spectrometers with an operating principle similar to that of photometers. The major difference is that the OPC optical sensing volume, formed by the intersection of a focused light beam with a narrow particle beam, is much smaller so that only one particle is illuminated at a time. The scattered light is detected by a photo detector as an electrical pulse. The particle size is determined from the pulse height using a calibration curve typically obtained from measurements with spherical particles of known size and composition. The lower detection size limit is above 100 nm so it cannot be used for size distribution in the lower nanoparticle range. For particles large enough to be detected, OPCs are capable of measuring concentrations of up to 103 cm-3 before coincidence errors become too large. A disadvantage of OPCs is that uncertainty in refractive index often leads to significant variability in derived size distributions, even for the ideal case of homogeneous spherical aerosol particles (Giechaskiel et al. 2014). This means that since an optical particle counter is sensitive to the shape and refractive index of the particles, the measured particle sizes and thus the number distributions are approximate (Wahlstom et al. 2010a). N6) Scanning Mobility Particle Sizer (SMPS) is used to measure number size distributions for particles in the mobility size range from 10 to 445 nm. It combines a differential mobility analyzer (DMA) for size classification along with an electrometer or a condensation particle counter (CPC) for the detection of the particles. The particles are charged in a controlled manner and then sequentially classified according to their electrical mobility. With the controlled charging, particle electrical mobility corresponds to particle size. The counter subsequently registers the particles in sequential size classes. The counter is a condensation nuclei counter which uses condensation to optically count particles down to 10 nm. A few inter-comparisons of size distributions with SMPS systems of the same or different manufacturers have shown differences of the size distributions of 10%. However differences of >20% can also be found, especially for non-spherical particles. Such differences can be attributed to differences in particle charging efficiency, CPC counting efficiency, diffusion losses and non-ideal DMA transfer functions. Despite the potential for variability, the SMPS is arguably the most accurate instrument for high resolution size distributions of diluted exhaust aerosols (Giechaskiel et al. 2014). Mass concentrations can also be calculated assuming a density of 1,000 kg/m3. N7) Electrical Low Pressure Impactor (ELPI) is a cascade impactor which classifies particles according to their aerodynamic diameter. It is used to collect second by second information on particle size distributions. The ELPI operates by using a corona discharge to charge the particles prior to their introduction into the cascade impactor portion of the instrument. This portion includes several stages with D50% cut points in the size range of 16.5 nm to 7 μm. As the particles within specific size ranges impact onto the corresponding stages, electrometers record the charge that is deposited. The resulting currents are converted to particle number concentrations by dividing by the charging efficiency, which depends on particle diameter, and correcting for particle losses on preceding stages. These, can also be converted to mass-weighted size distributions using an approximate value for the density of the particles. Integration over the size distribution gives the total number and mass of wear particles generated per test. ELPI is used quite often for research in engine tests beds and generally the agreement with the PM mass is within 10% for emissions in the range of non-DPF vehicles. At low emission levels the agreement is not so good due to the filter artefact. With other instruments (e.g. LII or PASS) the agreement at low levels (e.g. <3 mg/mi) is better than 10–20% (Giechaskiel et al. 2014). D. Chemical and morphology characterization C1) Electron microscopy methods provide a means to examine the sizes and morphology of particles. This applies mainly to solid particles since semi-volatile particles are difficult to detect because they evaporate under vacuum and heating by the electron beam. Scanning Electron Microscope (SEM) uses a focused beam of high-energy electrons to generate a variety of signals at the surface of solid specimens. The signals that derive from electron-sample interactions reveal information regarding morphology, chemical composition, and crystalline structure and orientation of materials making up the sample, but they yield no information about the compounds constituting the wear particles. This information is needed if we are to understand the chemistry of the wear particles (tyres and brakes) and estimate the temperature in the contact (brakes). The method has other disadvantages like the high time required for analyzing a sufficient number of particles in order to ensure statistical representatives. Also, care must be taken to interpret 3 dimensional shapes and sizes from the 2 dimensional images. SEM is usually coupled with Energy Dispersive X-Ray Spectroscopy (EDX) for chemical characterization of particles with diameters between 100-1000 nm (Österle et al. 2008). C1 Scanning Electron Microscope (SEM) Type of instrument Measurement Principle Output Measuring range What can measure Electron Microscope Electron interaction with visual detection SEM images of wear particles Not applicable Morphology and size of wear particles; Focuses on the sample’s surface and composition; Provides a three dimensional image; Appropriate for nanoparticles Quantitative analysis of elements; Organic compounds Method good to be combined with other methods (EDX or XRD or XRF) for quantitative analysis What cannot measure Main limitations C2) Transmission Electron Microscopy (TEM) uses high energy electrons which are accelerated to nearly the speed of light. When an electron beam passes through a thin-section specimen of a material electrons are scattered. A sophisticated system of electromagnetic lenses focuses the scattered electrons into an image or a diffraction pattern, or a nano-analytical spectrum, depending on the mode of operation. Each of these modes offers a different insight about the specimen. The imaging mode provides a highly magnified view of the micro- and nanostructure. The diffraction mode displays accurate information about the local crystal structure. Nano-analytical modes (x-ray and electron spectrometry) tell researchers which elements are present in the material. TEM has much higher resolution compared to SEM. Furthermore it is able to provide details about the internal composition of the sample. TEM is usually coupled with Energy Dispersive X-Ray Spectroscopy (EDX) or Energy Filtered (EF) system for chemical characterization of particles with diameters < 100 nm (Österle et al. 2008). C2 Transmission Electron Microscope (TEM) Type of instrument Electron Microscope Measurement Principle Output Measuring range What can measure What cannot measure Main limitations Electron interaction with visual detection TEM images of wear particles Not applicable Morphology and size of wear particles; Elemental composition; Appropriate for crystallites in the range of 21000 nm; Much higher resolution compared to SEM Quantitative analysis of elements; Organic compounds Method good to be combined with other methods (EDX or XRD or XRF) for quantitative analysis; Provides a 2 dimensional image C3) X-Ray Fluorescence (XRF) utilizes x-rays for qualitative and semi-quantitative inorganic chemical analysis of unknown samples. X-Rays bombard atoms in the sample and electrons are removed or ejected from inner shells. Electrons from outer shells of the atom drop down to fill the vacant position and to return the atom to a more stable, ground state. When this occurs energy is produced, some of which is in the form of X-Rays. Each element has its own unique X-Ray signature meaning that X-Rays from a sample can provide detailed information about it. The main advantages of XRF include easy sample preparation compared to other inorganic analysis methods, multielement determination (all elements between Na and U can be simultaneously analyzed), as well as the possibility to screen completely unknown samples. On the other hand, XRF provides qualitative analysis of elements without indicating the phases which are present in the sample, while quantitative analysis of elements is not very accurate. C3 X-Ray Fluorescence (XRF) Type of instrument Measurement Principle Output Measuring range What can measure Spectrometer X-Ray fluorescence energy detection Spectra of elements and quantification (counts/energy) Down to ppm concentrations for most elements All elements with atomic number greater than 11; Nondestructive method; Easy sample preparation; Possibility to screen completely unknown samples Organic compounds; Elements lighter than Na No information about the phases of the element present; Semi-quantitative method good to be combined with other methods (XRD) What cannot measure Main limitations C4) Energy Dispersive X-Ray Spectroscopy (EDX or EDS) is a variant of XRF which makes use of the Xray spectrum emitted by a solid sample bombarded with a focused beam of electrons to obtain a localized chemical analysis. All elements from Be to U can be detected in principle, though not all instruments are equipped for 'light' elements (Z < 10). High energy beam of charged particles may excite an electron in an inner shell, ejecting it from the shell while creating an electron hole where the electron was. An electron from an outer, higher-energy shell then fills the hole, and the difference in energy between the higher-energy shell and the lower energy shell may be released in the form of an X-ray. The number and energy of the X-rays emitted from a specimen can be measured by an energy dispersive spectrometer. As the energy of the X-rays is characteristic of the difference in energy between the two shells, and of the atomic structure of the element from which they were emitted, this allows the elemental composition of the specimen to be measured. EDX is usually coupled with SEM for chemical characterization of particles with diameters between 1001000 nm and allowing thus phase distinction (Österle et al. 2008). C4 Energy Dispersive X-Ray Spectroscopy (EDX or EDS) Type of instrument Measurement Principle Output Measuring range What can measure Spectrometer X-Ray dispersive energy detection Spectra of elements and quantification (counts/energy) Down to ppm concentrations for most elements All elements with atomic number greater than 10; Nondestructive method Organic compounds No information about the phases of the element present; EDX is usually coupled with SEM for phases characterization of particles with diameters between 100-1000 nm; Not all instruments are able to measure light elements (Z<10) What cannot measure Main limitations C5) X-Ray Diffraction Spectroscopy (XRD) is an instrumental technique that is usually used to study crystalline materials. Its main difference from XRF is that it can determine the presence and amounts of minerals species in sample, as well as identify phases. The three-dimensional structure of nonamorphous materials is defined by regular, repeating planes of atoms that form a crystal lattice. When a focused X-ray beam interacts with these planes of atoms, part of the beam is transmitted, part is absorbed by the sample, part is refracted and scattered, and part is diffracted. When an X-ray beam hits a sample and is diffracted, we can measure the distances between the planes of the atoms that constitute the sample by applying Bragg's Law. The characteristic set of d-spacings and theirs intensity generated in a typical X-ray scan provides a unique "fingerprint" of the phases present in the sample. When properly interpreted, by comparison with standard reference patterns and measurements, this "fingerprint" allows for identification of the material. XRD methods for crystallite size determination are applicable to crystallites in the range of 2-100 nm. The diffraction peaks are very broad for crystallites below 2-3 nm, while for particles with size above 100 nm the peak broadening is too small. Due to the complexity of XRD data analysis, the chemical composition of the sample must be known in advance by a semi-quantitative analysis (i.e. XRF) in order to accurately pin point the phases present in your sample. XRD is not good for organic materials, as they often have very similar signatures. Both XRD and XRF are non-destructive methods. C5 X-Ray Diffraction Spectroscopy (XRD) Type of instrument Measurement Principle Output Spectrometer X-Ray diffraction patterns for detection Spectra of elements and their phases and quantification (counts/energy) Measuring range What can measure All elements with atomic number greater than 13 and their What cannot measure Main limitations phases; Appropriate for crystallites in the range of 2-100 nm; Non-destructive method Elements with atomic number smaller than 13; Organic compounds Chemical composition of the sample must be known in advance by a semi-quantitative analysis C6) Proton Induced X-Ray Emission (PIXE) has the same operating principle as the previously described spectroscopy methods. In PIXE the incident beam particles (usually 3 MeV protons) eject inner shell electrons from the target atoms which results in the emission of characteristic X-rays. With a suitable x‑ray detector more than 70 elements with atomic number larger than 13 can be detected. PIXE is similar to EDX only with electron microprobes. However, due to the complete absence of primary bremsstrahlung the sensitivity of PIXE is enhanced by about a factor of 100 compared to EDX and is of the order of ppm for most elements. Quantitative analysis is also possible with the appropriate corrections to absorption and x-ray yields. PIXE is often used together with imaging nuclear microprobes for spatial elemental mapping. C6 Proton Induced X-Ray Emission (PIXE) Type of instrument Measurement Principle Output Measuring range What can measure Spectrometer Proton bombarding followed by X-Ray detection Spectra of elements and quantification (counts/energy) Down to ppm concentrations for most elements All elements with atomic number greater than 13; Higher sensitivity compared to other spectroscopy methods Elements with atomic number smaller than 13; Organic compounds No information about the phases of the element present; Has to be used with other techniques to gain information regarding the phases What cannot measure Main limitations C7) Thermal/optical carbon analyzer working principal is separated into two steps: first, the sample is heated in an inert atmosphere to volatilize organic material to CO2 or CH4. Carbon measured in this step is designated as Organic Carbon (OC). After that oxygen is introduced to the remaining sample and heated to higher temperatures (up to 900°C). The measured carbon in this step is designated as Elemental Carbon (EC). In this process, OC may char in an oxygen free atmosphere and erroneously be detected as EC. Some refractory OC may also be counted as EC. Finally, some EC may be counted as OC due to the activity of catalytic or oxidizing species adsorbed in the PM. Hence, the split between EC and OC with this method is not accurate. Different measurement protocols in terms of heating rate and oxidation temperature, as well as optical correction methods for charring may be used. Hence, the EC/OC split is operationally defined when thermal/optical analysis is involved. Inter-laboratory comparison studies show that different thermal methods agree within 5–15% on the total carbon (EC+OC) concentrations, but the EC and OC concentrations can differ by a factor of more than two (Giechaskiel et al. 2014). One important benefit of using thermal-optical carbon analysis is the availability of widely-accepted and extensively used calibration methods. C7 Thermal/Optical Carbon Analyzer Type of instrument Measurement Principle Output Measuring range Carbon analyzer Oxidation of PM and optical detection Flame Ionization Detector (FID) signal of CH4 quantification Down to ppm concentrations for both EC and OC (less than 1 μg/m3 for atmospheric samples) Elemental and Organic Carbon; Total Carbon Specific organic compounds; Inorganic compounds The split between EC and OC is not accurate; EC and OC concentrations can differ from the actual in a factor of 2 or more; Requires different filter for PM collection (quartz) What can measure What cannot measure Main limitations C8-C9) Inductively Coupled Plasma Mass Spectrometry (ICP-MS) and Inductively Coupled Plasma Atomic Emission Spectroscopy (ICP-AES) are analytical techniques used for the detection of trace metals and elements. In both techniques the sample is typically introduced into the ICP plasma as an aerosol where it is completely dissolved and the elements in the aerosol are converted first into gaseous atoms and then ionized towards the end of the plasma. Excited ions and atoms can be detected either by measuring the m/z ratio of the different ions formed (MS) or by measuring the electromagnetic radiation which is emitted at wavelengths characteristic of each element (AES). In both methods the sample has first to be digested. ICP-MS has detection limits for most elements equal to or better than those obtained by Graphite Furnace Atomic Absorption Spectroscopy (GFAAS). One advantage is the ability to handle both simple and complex matrices with a minimum of matrix interferences due to the high-temperature of the ICP source. Also ICP-MS has superior detection capability to ICP-AES with the same sample throughput, as well as the ability to obtain isotopic information. None of these techniques can be used for organic compound determination. C8-C9 Inductively Coupled Plasma – Atomic Emission Spectroscopy/Mass Spectrometry (ICP-AES/MS) Type of instrument Measurement Principle Output Mass or Atomic Emission Spectrometry Conversion to plasma & atomic emission or mass detection Spectra of elements and quantification (counts/mass) or (counts/wavelength) Down to ppb concentrations for all elements A wide range of metals and trace elements; Ability of handling both simple and complex matrices; High sensitivity and selectivity Organic compounds Requires difficult and time consuming digestion procedure; Expensive instrumentation; MS detection has superior detection capability to AES; MS analysis is much faster and multi-element compared to AES Measuring range What can measure What cannot measure Main limitations C10) GC-MS is an analytic technique which combines the separating power of Gas Chromatography with the detection power of Mass Spectrometry. MS is a wide-ranging detecting technique, which involves the production and subsequent separation and identification of charged species according to their mass to charge (m/z) ratio. Identification of chemical species is accomplished by matching both the gas chromatographic retention times to pure components and mass spectral fragmentation patterns to standard MS libraries. GC uses a carrier gas to transport sample components through either packed columns or hollow capillary columns containing the stationary phase. In general GC columns have smaller internal diameter and are longer than HPLC columns. GC-MS is used for determination of organic compounds of wear particles. In this method the sample has first to be extracted through a difficult and time consuming procedure. Aatmeeyata et al. (2010) proposed the following temperature program for PAHs separation: initial temperature of 70 °C (4 min), heated to 150°C at 15°C min−1, then to 210°C at 3°C min−1, then held at 210°C (8 min), and finally heated to 290°C at 2°C min−1 (5 min). GC-MS presents lower sensitivity for PAHs detection compared to HPLC techniques coupled either with UV or FLD. C10 Gas Chromatography Mass Spectrometry (GC-MS) Type of instrument Measurement Principle Output Measuring range What can measure What cannot measure Main limitations Gas Chromatography Column separation followed by mass detection Chromatogram of organic compounds and quantification Down to 10 ng/ml for most PAHs Full range of organic compounds Requires difficult and time consuming extraction procedure; Lower sensitivity for PAHs compared to HPLC C11) High Performance Liquid Chromatography (HPLC) is an analytical method that yields high performance and high speed compared with traditional column chromatography. It has the same operating principle as GC with the major difference being at the sample condition during separation (liquid instead of gas). It is based on the principal that under the same conditions, the time between the injection of a component into the column and the elution of that component is constant. Fluorescence detector (FLD) is probably the most sensitive among the existing HPLC detectors. Typically, fluorescence sensitivity is 3 orders of magnitude higher than that of the UV detector for strong UV absorbing materials. FLDs are very specific and selective among the others optical detectors. This is normally used as an advantage in the measurement of specific fluorescent species in samples like for example PAHs. HPLC-FLD has been used for determination of PAHs in tyre wear particles with higher sensitivity compared to GC-MS. C11 High Pressure Liquid Chromatography Fluorescence Detector (HPLC-FLD) Type of instrument Measurement Principle Output Measuring range Liquid Chromatography Column separation followed by fluorescence detection Chromatogram of selected PAHs and quantification Down to 0.02 ng/ml for most PAHs What can measure What cannot measure Main limitations Organic compounds that fluorescence (PAHs); Higher sensitivity compared to other detectors Compounds without fluorescence radiation Requires difficult and time consuming extraction procedure
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