A.1.1 Definition of strains.
In our analysis the PVDF foil is treated according to the Kirchhoff–Love plate theory, which reduces a three-dimensional plate to the mid-surface plane of its two-dimensional representation. It includes the following assumptions:
• the foil is thin, i.e., its thickness h is much smaller than its radial dimension a; in our case this assumption is fulfilled well, the thickness-to-diameter ratio h/(2a) ranges from 8.3 × 10−4 to 25.0 × 10−4
• the foil thickness is constant, i.e., not affected by the impact of the particle jet
• mechanical deflections of the foil are small, such that Hooke's law applies, i.e., the deflection is proportional to the mean force exerted by the impinging particles
• lines normal to the mid-surface remain normal to the mid-surface when deformed, see Fig. 9.
 |
| Fig. 9 Schematic sketch of an elastically mounted PVDF foil in the rest (grey lines) and deflected (red lines) position. The axial and radial displacements w(r,t) and u(r,t), respectively, are indicated. The axial displacement is given by the distance between the undeformed mid-surface (dashed grey line) and the deformed mid-surface (dashed red line). The radial displacement correlates with the derivative of the axial displacement. The z-axis corresponds to the beam axis. | |
For a circular foil cylindrical coordinates are appropriate – these are the radial coordinate r, the tangential coordinate θ and the axial coordinate z. The centre position of the foil is the origin of the coordinate system. Accordingly, Sr and Sθ are mechanical strains in radial and tangential direction, respectively; both are caused by the elongation of the foil. The strain according to a compression is Sz, but because the thickness of the foil is assumed to be constant, Sz equals zero.
The PVDF foil is polarized in the direction of the axial axis. The axial component of the electric field
z, however, equals zero because the PVDF foil is virtually grounded by the amplifier, see Fig. 4. Therefore, the electric displacement in z-direction according to eqn (1) is given by:
|
 | (2) |
The parameters e can be written as the product of the piezoelectric constants d and the stiffness coefficients,
. Because only very small deflections occur, e.g., in Fig. 11 less than 35 μm for He and less than 20 μm for Ar, anisotropy is neglected and the stiffness coefficients
of an isotropic material are used and expressed by Young's modulus Y and Possion's ratio μ: |
 | (3) |
The piezoelectric constants d31 and d32 are equal, because the used PVDF foil is stretched biaxially. Hence, the amount of generated surface charges q can be calculated by applying Gauss's law: |
 | (4) |
Eqn (4) is integrated over the effective, sensitive detector area A = a2π, where a is its radius. As current is the change of charge per time, the current is: |
 | (5) |
The deflection is described by the displacement fields u(r,θ,z,t), v(r,θ,z,t) and w(r,θ,z,t) in the radial, tangential and axial directions, respectively. They are all related to the axial displacement, see Fig. 9, given by:23
|
 | (6) |
Only axisymmetric vibrations are considered and thus w is independent of θ and the tangential displacement field v equals zero. Accordingly, the strain components for small axial displacements are:
|
 | (7) |
A.1.2 Driven vibration of a circular PVDF foil.
The axial displacement of a circular thin membrane due to vibration can be described by:24 |
 | (8) |
Here, D is the tension of the membrane, ρ the density of the PVDF foil, m the mass of the vibrating system and F the force applied on the PVDF foil. For simplicity, the radial particle distribution is approximated as being uniform, not depending on the radial position, allowing to derive an analytical solution. The damping of the vibration is described by the term −2ξdw/dt, with ξ a damping constant. In order to solve the differential equation eqn (8), w(r,t) is separated into a spatial part, Wl(r), and a temporal part, Zl(t), for every vibration mode l. Accordingly, the axial displacement for all l modes is given by:
|
 | (9) |
For the radial part, the solution of the harmonic case is assumed:
|
 | (10) |
Jk are the Bessel functions of the first kind of the kth order and cl are the normalization constants. The boundary conditions are given by the requirement that the deflection is zero at the edge:
This is fulfilled if the roots λl are given by:
There exists an infinite number of roots and, thus, an infinite number of eigenfrequencies. The normalization constants cl are calculated via:
|
 | (13) |
The temporal parts Zl(t) are computed using eqn (9) and (10) substituted in eqn (8) |
 | (14) |
provided that the force F is defined via the normalized integral of the forces fl(t) of all vibrational modes: |
 | (15) |
The eigenfrequencies ωl are given by: |
 | (16) |
Therefore, the tension of the membrane can be accessed by determining the eigenfrequencies. In order to proof our assumptions (membrane vibration, consideration of axisymmetric vibration only) frequency spectra for different detector sizes are calculated from measured PVDF detector signals and shown in Fig. 10. Obviously, the observed vibration frequencies of the PVDF foil match the ratios expected from our model description rather well. It thus may be concluded that both assumptions are fulfilled for the detector with a sensitive radius of 5 mm. The frequency spectrum of the detector with a sensitive radius of 15 mm also shows interfering signals and many non-axisymmetric vibrations. If the supersonic jet is interrogated on the symmetry axis and at distances where particle–particle collisions have ceased, the one-dimensional Maxwell–Boltzmann velocity distribution is effectively indistinguishable from a shifted Gaussian distribution.25 Therefore, the time dependence of the applied force fl(t) of the lth mode is given by:
|
 | (17) |
Here, fl,max is the maximum applied force of the lth mode, t0 is the mean arrival time of the incoming particle pulse, and σ is a measure of the temporal width. The maximum applied force is related to the average force
l and can be determined by the full width at half maximum (FWHM): |
 | (18) |
The time dependence of the axial displacement Zl(t) is given by eqn (14) and can be calculated analytically: its solution is obtained by the Fourier transform of eqn (14). The inverse Fourier transform results in: |
 | (19) |
Here, ω is an angular frequency and Re[x] gives the real part of x.
is given by: |
 | (20) |
Eqn (19) can be rewritten as:26 |
 | (21) |
with
and a dummy integration variable t′. Eqn (21) can be evaluated by a computer algebra system such as Mathematica.
 |
| Fig. 10 Frequency spectra calculated from the measured time spectra for two different detector sizes. The good agreement between the experimental and theoretical values supports the applicability of the model assumptions. The theoretical multiplies of the frequency λl/λ1 for different k are calculated by the ratio of the roots given by Jk(λl). In the case of k = 0 the vibrations are axisymmetric, for k ≥ 1 the vibrations are non-axisymmetric. The uncertainty of the frequency determination can be estimated by a comparison with a known frequency such as the frequency of the turbo molecular pump (660 Hz, marked with an asterisk). From this, the uncertainty of the frequency is estimated to be in the range of ±2.3%. | |
A.1.3 Applied mean force of a supersonic jet on a surface.
The change of the momentum of particles colliding perpendicularly with a surface within a certain time, dt, results in a force onto the surface which is given by: |
f(t)dt = d(mpulse ) | (22) |
Here, the momentum mpulse
is given by the mass of all impinging particles, mpulse, multiplied by the mean particle velocity,
. The duration of the surface collision tFWHM is approximated by the FWHM of the impacting particle pulse. The integration of eqn (22) over time yields the time-average of the force
: |
 | (23) |
The momentum change depends on the change of the particle velocity, which can be described by the coefficient of restitution, κ, with 0 ≤ κ ≤ 1: |
 | (24) |
κ and thus
depend on the gas–surface interaction with: |
 | (25) |
The mass of all impacting particles is related to the average particle density, ρpulse, seen by the detector |
mpulse = ρpulsesFWHMA | (26) |
where sFWHM is the distance the particle jet travels in the time tFWHM: |
sFWHM = tFWHM![[v with combining macron]](https://www.rsc.org/images/entities/i_char_0076_0304.gif) | (27) |
As already noted in Section A.1.2, the density is assumed to be constant over the detector area. Using eqn (22), (25) and (27), the mean force applied by impacting particles in a pulsed, supersonic molecular beam experiment is expressed by the momentum flux of the impacting particles and the sensitive detector area A: |
= (1 + κ)ρpulse 2A | (28) |
A.1.4 Generated current due to vibration.
The current generated by the displacement of the PVDF foil can be calculated using eqn (5) with the definitions of the strains, eqn (7), and the axial displacement w(r,t), which is given by eqn (9) and its solution according to eqn (10) and (21). Because the strain depends on the z-position, the average strain is calculated by integration of eqn (5) from w(r,t) to w(r,t) + h/2 and standardized by multiplication with 2/h. Because the axial displacement w(r,t) is small, the integration limit can be simplified to the range from 0 to h/2. The integration over half the thickness of the foil is due to the opposite charge generation: +q|z=h/2 and −q|z=−h/2.