Pacific Nanotechnology Inc.
An introduction to Atomic Force Microscopy Modes
Paul West and Arthur Ross
Introduction
The Atomic Force Microscope (AFM) is a scanning probe imaging and sensing device, useful for
physical and chemical studies. In its basic configuration, it measures the microscopic surface profile
of a near-planar target by mechanically scanning a tiny probe across it in a raster pattern. The
probe rises and falls in accordance with the surface profile. As it does so, its position is sensed and
captured digitally. That captured topogram can then be rendered as a photograph-like image,
reminiscent of an optical micrograph.
Although the AFM is but one of a family of scanning probe "microscopes" (see Table 1) the
AFM is far more versatile and capable than the others, viz:
The three dimensional profile of a surface is measured with the AFM by monitoring the position
of the probe in three dimensions as it scans. A feedback control system maintains the force
between the probe and the surface sensibly constant during the scan. The probe tip thus follows
the surface profile, as one might do with a finger tip at a more macroscopic scales.
Soon after the invention of the AFM it was realized that these instruments were capable of measuring
far more than surface topography. It is possible to measure any physically phenomenon at
the nanometer scale for which a suitable sensor can be incorporated in the probe. Demonstrated
examples include magnetic fields, electric fields, contact potential difference, temperature, and
hardness. It is also possible to use the AFM probe as a tool to modify surfaces.
Such non-topographic uses have come to be called AFM "modes". It is the purpose of this monograph
to elaborate upon these modes, both in principle and in practice.
.
AFM "Modes"
This is a white paper on AFM modes. There's a problem with the notion of "modes", as this is
really a misnomer. The "mode" terminology is, however, deeply entrenched amongst workers in
this exciting field as a sort of shorthand name for one of the myriad AFM techniques or applications.
Therefore, with an English teacher's caveat regarding possible bad usage, we present the list
in Table Table 2: as a practical user's map.
AFM Basic implementation
Figure 1-1 shows the elements of a basic atomic force microscope. The probe tip is positioned in
three dimensions by three mutually orthogonal actuators. Each actuator is a
piezoelectric ceramic
transducer
(PZT). PZTs are well suited to the small motions required by the AFM. Their travel is
approximately linear in the applied voltage when used in the AFMs.
We adopt the convention that the X and Y coordinate axes are nominally parallel to the
surface
under test
(SUT), and the Z axis completes a right handed Cartesian coordinate system. The Z
axis positioner thus moves the probe toward (negative Z) or away (positive Z) from the SUT,
while the X and Y positioner move the probe in a nominal object image plane. In normal operation,
the X and Y position is programmed in a raster scanning path, while the Z position is tightly
controlled relative to the SUT by a feedback control loop. The Z-axis error signal is derived from
a force transducer that measures the force on the probe tip. The transducer output is differenced
against a fixed voltage, which corresponds to a setpoint (target) force. The error signal is amplified
and drives the Z-axis PZT. This control loop acts to reduce the error signal, and hence the probeto-
SUT distance to near-zero. The feedback loop thus causes the probe to closely follow the
undulations of the SUT while the X-Y PZTs scan the probe over a rectangular image area. Meanwhile,
the control voltage applied to the Z-PZT provides a convenient representation of the elevation
of the probe and surface is used to generate and image or topogram of the surface.

Light lever force sensing
High sensitivity in the force transducer of an AFM can be achieved by a simple geometric optical
device known as the light lever (see Figure 1-2). A low-power laser beam is reflected from the top
of the cantilever to a distant photo detector. Small displacements of the cantilever result in large
displacements of the laser beam at the location of the detector due simply to the large "lever arm"
of the light path. The detector is bifurcated, and the halves are differenced, giving a force-proportional
error signal.

Probe-surface interactions
While it might be thought that the force between an AFM probe and a hard surface might have
an abrupt brick wall character, this is an over-simplification at the nanoscopic scale. Not only are
fundamental interatomic forces finite in extent, there is also the problem of surface contamination.
AFMs are usually operated in ambient environmental conditions (room temperature, atmospheric
pressure, ambient air). As a result, there is invariably a surface layer comprised of water
and miscellaneous hydrocarbons. This layer is thick enough relative to the nominal probe operating
height that the probe tip is almost always immersed in it (Figure 1-3).
The forces between probe and surface, to the extent that they are position-dependent only, i.e. are
lossless, can be represented by an effective potential energy (see, for example, Figure 1-4)
As shown in Figure 2-9, the interaction between probe and surface falls into one of three zones:
There are two primary methods for measuring the force between a probe and a sample: contact
mode and vibrating mode.
Contact mode entails a direct quasi-static force versus distance measurement, that is, a rather intimate
contact between probe and surface. While producing accurate results, it tends to rapidly
damage both probe and surface.
Vibrating mode may be either large amplitude, in which the probe contacts the surface on every
cycle, or small amplitude non-contact. The latter is generally less stressful on both the probe and
surface, and tends to give superior results. It measures more subtle properties of the surface.
Principles and Components

As originally conceived, the AFM (see Figure
2-1) was a surface profiling device. A nanometer-
scale probe, mounted at the end of a tiny
cantilever, is held in contact with the surface
using piezoelectric positioning. Deflection of
the cantilever, easily measured optically, indicates
force between probe and surface. That
force is held nominally constant by a feedback
control system while the probe is scanned raster-
fashion across the surface. The control voltage
indicates elevation as a function of
transverse position. The elevation can be displayed
or recorded in various ways, providing a
topogram of the surface. The resolution, limited
by the probe tip radius, is of the order of a few
tens of nanometers, with fields-of-view of the
order of a few tens of microns.
Subsequent to those original demonstrations, many variations on this basic design have been developed. Oscillatory sensing was introduced for improved performance and for field gradient
sensitivity. While all of them measure cantilever deflection as a positioning aid, the feedback control
error signal can be derived in several ways. And exactly what constitutes a surface "profile" can
be defined variously, depending upon ones objectives.
This chapter described the basic AFM instrument and some of its possible variations.
Coordinate system.
We adopt the convention that the X and Y coordinate axes are nominally parallel
to the surface under test (SUT), and the Z axis completes a right handed Cartesian coordinate
system, as shown in Figure 2-1. The Z axis positioner thus moves the probe perpendicular to the
SUT, while the X and Y positioner move the probe in a nominal object image plane.
Topography by quasi-static probe contact
In contact mode, the cantilever is scanned over a surface at nominally constant force. The Z axis
PZT feedback loop, if properly implemented, ensures near constancy of cantilever deflection,
which corresponds to constant force.
Contact mode is typically used for scanning hard samples and when a resolution of greater than
20 nanometers is required. The cantilevers used for contact mode are usually silicon or silicon
nitride. Typical resonant frequencies are about 50 KHz and force constants are below 1 N/m.

Probes
AFM probe-cantilevers assemblies are readily available from commercial vendors. They are generally
made of silicon or silicon nitride, taking advantage of the highly-developed techniques of
micro lithographic for fabrication. Figure 2-3 shows SEM images of some representative tips.
The sharpness of the probe is a primary determinant of the resolution of the AFM. Probe tips are
approximately spherical, and are characterized by an effective radius. A typical probe radius is in
the neighborhood of 10-20 nm. Special "supersharp" tips of even smaller radii, approaching 1 nm,
are offered, these being more suitable for probing narrow structures.
Probe coatings.
Probes are often used with various coatings for sensing particular phenomena. For
use with the light lever detection system, the cantilever backside is aluminized for high optical
reflectivity. Available probe coatings include:
Figure 2-4 shows some SEM images of probe tips at very high magnification.
Cantilever stiffness
For small deflections of the probe relative to its equilibrium (non-contact) position, the force versus
distance characteristic is, to a good approximation, linear. The force can thus be approximated
by Hooke's law:
Because of the strong analogy to the simple mass-spring oscillator so familiar from elementary
physics classes, we will often call k the cantilever "spring constant", tho the terminology is not rigorously
appropriate.
k can be calculated if the dimensions and composition of the cantilever are known. Most commercially
available cantilevers are supplied with a value for k , but these are often unreliable. For best
results, Sader's method is recommended. The length and width of the cantilever are measured
with an optical microscope and an approximate mechanical Q is measured by scanning the excitation
frequency while observing the mechanical response. From those the effective spring constant
can be calculated.
Lateral compliance

As illustrated in Figure 2-5 the
cantilever in an AFM can bend,
and twist as it is scanned across a
surface.
The horizontal forces are dependent
upon the so-called "asperity"
of the surface (its abrasive
nature) relative to the probe, that
is, the sliding friction between
probe and surface.
Typically the compliance for
twisting is much less than the
compliance for bending. The
twisting sensitivity, of course, is
to the forces that exert a moment
around the cantilever's major
axis, that is, forces perpendicular
to the axis of the cantilever and
parallel to the SUT.
Probe position sensing
Light lever.
High sensitivity in the force transducer of an AFM can be achieved by a simple geometric
optical device known as the light lever (see Figure 2-6). A low-power laser beam is
reflected from the top of the cantilever to a distant photo detector. Small displacements of the
cantilever result in large displacements of the laser beam at the location of the detector due simply
to the large "lever arm" of the light path.


Position sensitive detector.
Cantilever torsion
is measured by an enhancement of the light
lever. A four-quadrant
position sensitive detector
(PSD) is used with the signals added and
subtracted as shown in Figure 2-7 to give
equivalent vertical and horizontal displacements.
Because the vertical and lateral
deflections are substantially independent of
one another, it is possible to measure topography
and lateral friction force independently
(see §). Because the physical
dimensions of commercially available cantilevers
are not well characterized, the elasticity
coefficients must be calculated
individually for each cantilever from measured
dimensions and material properties.
Optical interferometry.
Some practitioners have used optical interferometry on the cantilever for
extreme sensitivity to Angstrom-scale deflection (see, for example, Martin et al, (1987) for a heterodyne
technique, Erlandsson et al, (1988) for non-heterodyne). While the potential sensitivity
of interferometry is higher (sub-A) than that of the light lever, its cost and complexity discourage
its use for all but the most demanding applications.
Probe-surface interactions
While it might be thought that the force between an AFM probe and a hard surface might have
an abrupt brick wall character, this is an over-simplification at the nanoscopic scale. Not only are
fundamental interatomic forces finite in extent, there is also the problem of surface contamination.
AFMs are usually operated in ambient environmental conditions (room temperature, atmospheric
pressure, ambient air). As a result, there is invariably a surface layer comprised of water
and miscellaneous hydrocarbons. This layer is thick enough relative to the nominal probe operating
height that the probe tip is almost always immersed in it (see Figure 2-8), forming a meniscus
that complicates near-surface operation.

The forces between probe and surface, to the extent that they are position-dependent only, i.e. are
lossless, can be represented by an effective potential energy (see Figure 2-9).

There are three basic regions of interaction between the probe and surface:
Piezoelectric transducer (PZT) positioning The X-Y resolution of the measurements possible in an AFM are of the order of the tip radius,
which is typically are a few tens of nm, and can be as small as just a few nm. If one postulates an
image area of 1000 x 1000 pixels (a rather high resolution digital image), at, say, 20 nm per pixel,
then the actual imaged area is 20
µ
m by 20
µ
m. This is far too small for simple mechanical positioning.
A far better solution is the use of piezoelectric ceramic positioners.
Piezoelectrics are materials that expand or contract in the presence of internal voltage gradients
(that is, bulk electric fields). The magnitude of the piezoelectric phenomenon makes these devices
quite appropriate as nanometer-scale actuators (see, for example, Gallégo-Juarez (1989)). Piezoelectric
actuators can produce, under electronic control, extremely fine position control down to
the nanometer scale required by an AFM. The motion is smooth, with no thresholds or "stickiness"
characteristic of electromechanical devices. The are non-magnetic, making them suitable for
applications that are magnetic-field sensitive. They are also capable of extremely high accelerations,
as much as thousands of
g
's, in combination with high forces, upwards of thousands of newtons.
There is no observable mechanical wear, in most applications.
Traditionally the PZT positioning in AFMs is done by a one-piece tubular actuator. Four electrodes
in a quadrant configuration cover the outside, while a full-circumference electrode covers
the inside. Voltages applied to opposite quadrant pairs causes tilt along the axis of symmetry.
Simultaneous voltage on all four quadrants causes elongation or contraction. The major virtue of
this design is its mechanical simplicity: one instrument provides motion in all three coordinate
axes. It does, however, have some drawbacks:
Of these, the most objectionable is perhaps the scan rate limitation. Achievable rates in typical
units are so slow that a full frame scan can take many minutes. Various speedup schemes, such as
the dual feedback controller scheme of Egawa et al (1999) have been tried, with mixed success.
This particular scheme used, as have others, a supplementary PZT actuator on the cantilever, in
addition to the principal tube-style 3D actuator. This sort of dual actuator configuration is especially
applicable to vibrating cantilever mode (VCM). The PZT tube actuator provides coarse Zaxis
positioning, but with slow dynamics, while the cantilever actuator provides fast, fine-grained
dynamics for both Z-axis positioning and cantilever drive.
The Proportional-Integral-Differential (PID) Feedback Controller.
Most AFM schemes for generating topography images make use of some sort of feedback control
system in conjunction with their error measurement and Z-axis actuator. The design and implementation
of such a feedback control system is non-trivial. The design is driven by unavoidable
trade-offs between tracking accuracy, speed, and stability. The simple, naive design will almost
always result in instability, entailing not only failure to track properly, but also damage or destroy)
the probe and sometimes damage the SUT. While a simple solution is possible, optimized solutions
require considerable sophistication in both analysis and implementation.
The AFM, when tracing SUT topography, might be regarded as a special case of the age-old
generic process control model shown in Figure 2-10 (upper).
The traditional industrial process control mechanism for a poorly-defined and/or inherently nonlinear
process is the so-called proportional-integral-differential (PID) controller. With reference to
Figure 2-10, the process drive y (
t
) is generated as a sum


Such a control mechanism is easily analyzed using LaPlace transforms and well-known techniques
if the overall system, that is the "plant" plus feedback amplifier, is linear and time invariant.
In the case of the AFM, however, the probe plus cantilever plus PZT actuator system is only
approximately linear. Moreover, even the dynamics in the linear approximation are not easily
characterized. Cantilever resonances are usually at tens of kHz and unimportant in topography
following. The typical tubular PZT actuator, however, has resonances in the neighborhood of a
few kHz. These are significant and do affect topography tracking.
The goals of the feedback controller design are straightforward:
The first and second of these are generally trade-offs against one another. Arbitrarily tight following
can be accomplished at the expense of extremely slow transient response, that is, of low closed
loop bandwidth. Rapid scanning can be achieved at the expense of large tracking error. The tradeoff
is, of course, a consequence of the stability requirement, which is absolute. A loop is either stable
or unstable, the latter being intolerable.
The usual solution in the practice of AF microscopy is to tune the PID coefficients semi-heuristically.
Such techniques are well-established in the literature of industrial process control. While
they do result in a stable system, its bandwidth is not large, thus limiting the usable scan speed.
Scanning speed is an especially important issue. AFMs using a simple PID style of feedback controller
can take many minutes to complete an image.
As noted above, the limiting factor in the loop design is usually the PZT actuator, which usually
has internal mechanical resonances in the neighborhood of a few khz. This is orders of magnitude
slower than the cantilever resonances. The cantilever itself thus is generally not significant in limiting
the closed loop bandwidth.
Schitter et al. (2001), recognizing the importance of the PZT in limiting system performance,
carefully characterized their PZT actuator dynamics through the mathematical tool known as system
identification. System identification is the creation of a linear system model using only observations
of input and output, rather that physical modelling. This is especially useful for the PZT,
physical modelling of which would be a very complex mathematical problem. System identification,
on the other hand, is relatively simple, producing directly a useful pole-zero model.

Using that model Schitter et al. then generated a controller
using the H
∞ control system criterion (see, for
example, Skogestad and Postlethwaite (1996)). This
design was implemented, and displayed significant
improvement in transient response (Figure 2-11).
Details of this sort of analysis and design are beyond
the scope of this paper, but they are well-known and
are documented in modern control theory textbooks
(e.g. references found in the Schitter et al. (2001)
paper).
Subsequent sections of this paper show a simple "feedback
amplifier." These should always be understood as
the classic PID controller, with the proviso that more
sophisticated designs may yield substantial performance
improvements.
Observing the Elevation. Note in Figure 2-10 the presence
of an elevation estimator whose inputs are the PZT control voltage and the cantilever deflection.
This is a correction that is required of all AFM feedback schemes, though we may, for
simplicity, omit it in system diagrams. The reason is simple. Even if we assume that we know the
actuator position with complete precision, the actual position of the probe tip is the sum of that
actuator position and the cantilever deflection. That is to say, the actuator sets the equilibrium
position of the probe, while the surface interaction deflects the probe away from that equilibrium
position. One must add (or subtract, depending on mechanical design details) the two to obtain
the true probe tip position. In more sophisticated designs, that is, ones that account for the PZT
dynamics, one must also account for the fact that the actuator position lags its control voltage
because of the mechanical resonances. While we will, in subsequent sections, show the amplifier
output as an analog of position, suitable for recording, this is an over-simplification if one is trying
to do precision work.
Quasi-static (QS) operation
"Quasi-static" here denotes operation where the relationship between applied force and displacement
is not significantly affected by inertia (mass) of the probe; the probe position thus represents
only a static force balance. "Quasi" is prefixed to show that probe motion is possible, tho scanning
is slow. Such operation is primarily applicable to surface following.
"Contact mode" might be considered to be simply a high-force form of quasi-static operation,
though all QS operation is not necessarily contact mode. Care should be used in reading too
much into the terminology, as it is often used loosely.
A typical quasi-static system architecture is shown in Figure 2-12. A feedback control loop
adjusts the equilibrium probe position so that the deflection matches a setpoint, thus keeping the
force constant. The actuator control voltage thus represents the surface profile as defined by constant
static force. That profile may vary slightly, depending on the exact value of the setpoint and
the steepness of the force profile.
A Q-S topogram may be generated simultaneously with measurements of specific physical surface
properties, or it may be itself the primary objective.
Vibrating Cantilever Mode (VCM)
In order to make more sensitive measurements, requiring better signal/noise ratios, in scientific
instruments it is common to modulate the signal being measured and use phase or amplitude
detection circuits. Use of modulated techniques shifts the measurement to a higher frequency
regime where there is less 1/f noise. Vibrating probes also can be sensitive to near-surface force
gradients, such as arise from surface polarization or magnetization.
In the AFM, the probe is vibrated as it is scanned across a surface. As shown in Figure 2-13, the
probe is vibrated in and out of surface potential. The modulated signal can then be processed with
a phase or amplitude demodulator.

The cantilever oscillatory excitation is normally provided by a piezoelectric ceramic, similar to
those used for X-Y positioning.
A typical vibrating system architecture is shown in Figure 2-14. The Z-axis position of the probe

is the sum of a fast oscillating drive component and a slowly-varying average position that is controlled
by a feedback control system. The feedback system adjusts the Z position of the SUT in
accordance with the error relative to a setpoint. The measurement which is compared to the setpoint
is amplitude, frequency, or phase, depending on the particular mode of operation in use.
Care is needed in the detailed design of the low pass filter and feedback control system, as there is
a potential for instability. That instability, moreover, is sensitive to details of the probe-surface
force relationship. A system that is stable for one value of setpoint can become unstable for a different
value of the setpoint. (The mathematics of this design are beyond the scope of this paper.)

Probe-cantilever dynamics. Vibrating modes all
make use of the natural mechanical resonance of
the probe-cantilever system. For most purposes
of AF microscopy, these dynamics can be adequately
modelled by a simple damped massspring
system (Figure 2-15). The mass and
spring identify readily with the actual mass and
stiffness, tho the physical source of the damping
is not entirely obvious. Such a system displays
the familiar Lorentzian resonance (Figure 2-16).
The amplitude response is


It is noteworthy that the amplitude at resonance

can be written
where

is the quasi-static amplitude response, that is, the amplitude that would result
if the force acted only against the spring. The amplitude on-resonance is thus enhanced by a factor
of

. This is, of course, the low frequency limit of (2-4). Also noteworthy is the exact
90° phase at resonance, that is, the displacement response lags the driving force by 90°.
Probe interaction with surface. When the probe tip interacts with a surface, the resonance frequency
generally shifts to a lower value, and there is a corresponding change in the phase. When scanning
in the vibrating modes, a constant relationship is maintained by the feedback electronics, which
keeps either the phase shift or amplitude constant at a given frequency, while scanning.
As discussed above, there is a contamination layer on surfaces in ambient air with a thickness
between 1 and 50 nanometers. Capillary forces, which are attractive, strongly affect probe behavior
near the contamination layer.
The probe may be used in three fashions as it is scanned across the surface (see Figure 2-17).

Regime 1 - The probe is vibrated across the surface of the contamination layer. The vibration
amplitude must be very small and a very stiff probe must be used. Typically, the images of the
surface contamination layer are very "cloudy" and appear to have low resolution. This is
because the contamination fills in the nanostructures at the surface.
Regime 2 - "Near Contact Mode" - The probe is scanned inside the contamination layer.
Very high resolution images can be produced by this technique, but great care is required. The
cantilever must be stiff so that capillary forces do not snap the probe to the surface, and the
amplitude must be very small.
Regime 3 - "Intermittent contact" or "tapping" mode - The probe is vibrated in and out of the
contamination layer. The energy in the vibrating cantilever is much greater than the depth of
the capillary attraction potential well. The probe thus moves easily in and out of the contamination
layer. This mode is conceptually simple, and is the easiest to implement, but it often
results in broken probes due to the surface crashes that occur on every cycle.
A side benefit of vibrating modes is that "stickiness" due to friction ("lateral") forces, if any, tends
to be released on each cycle as the probe moves away from the surface.
Typically, vibrating methods are used when the highest resolution is required or if very soft samples
are being scanned. The probes used for vibrating mode are often less than 10 nm in diameter.
Small amplitude VM topography. While both QS topography and VM topography use force feedback,
VM can operate at a much smaller force than QS, and operates in a fundamentally different
way.

Though the interaction force vs. displacement relationship
is fundamentally nonlinear, for sufficiently small displacements
it can be considered approximately linear, as
shown in Figure 2-18. Moreover, an approximate straight
line force relationship, tangent to the actual force curve, is
equivalent to a linear spring, whose stiffness
Δ
k = -Δ
F/Δ
A That equivalent spring adds to or subtracts
from the basic cantilever elasticity, altering keff.and
thus its resonant frequency. The shift is up in a repulsive
regime (larger
keff ), or down in an attractive regime
(smaller
keff ). Although the magnitude of the change can
be quite small, it is readily detected due to the generally
high Q of the resonance. Viscous losses in the SUT may also affect the parameters of the resonance, though the specific relationship is less obvious, and
generally is quite small compared to the elastic force contribution.
Any of several techniques can be used to detect the resulting change in the resonant frequency,
changes in amplitude and phase being most common.
When scanning in vibrating modes, a constant relationship is maintained by the feedback electronics,
which keeps either the phase shift or amplitude constant at a given frequency, while scanning.
Typically, small amplitude vibrating methods are used when the highest resolution is required or if
very soft samples are being scanned. Some examples are shown in.Figure 2-19


The probes used for vibrating mode are often less than 10 nm in
diameter. As vibrating mode imperils the probe more than simple
contact modes, it is prudent to periodically check its integrity with
a resolution reference sample that contains fine-scale features,
such as that shown in Figure 2-20.
Large amplitude VM topography. Large amplitude VM, often called
"tapping", is conceptually simpler than small amplitude VM, and
easier to implement. It has the advantage of being less affected by
the surface contamination layer. The probe is detached from the
surface meniscus on every cycle. As the effects of the surface on
the probe motion is more dramatic than in small amplitude VM, it
is more easily extracted from the deflection signal. It has disadvantages,
however:
The system architecture for large amplitude VM is essentially the same as small amplitude VM.
As before, care is needed in design of the feedback control amplifier that positions the SUT in the
Z coordinate, as there is a hazard of instability. The design is complicated by the fact that the
value of the coordinate setpoint can change the small-signal gain, thus altering the stability properties.
Force Gradient Modes
Nanoscopic-scale electrostatic and magnetostatic material properties are particularly accessible to
AFM measurement. Any interaction force for which a suitable probe exists can be mapped. The
mechanism of the mapping is the spatial gradient of the force. That spatial gradient adds or subtracts
from the effective spring constant of the AFM cantilever, as discussed above. The resulting
changes in resonant frequency are readily measured. The fields are sensed through the changes in
probe-cantilever resonance as the probe is moved slowly above the SUT.
Principles. For very small displacements of the probe, the z-axis gradient of the force modifies the
effective spring constant of the cantilever as discussed above. Assuming that the field, and thus
the force, varies only with Z, then the resonance of the probe-cantilever system is approximately:

and we have implicitly assumed that the force can be adequately modeled by the first term of its
Taylor series expansion in ΔZ.
(The negative sign arises because
F = -
kZ for a simple mass-spring oscillator.)
The shift in resonant frequency is sensitive to the first spatial derivative of the spring constant,
and thus to the second spatial derivative of the force, that is:
Measurements of the resonant frequency at two elevations thus yields an approximation to the
second derivative of the surface field strength.
Force gradient instrumentation techniques. Several schemes are used for such measurements:
Application to permanently polarized materials. The force gradient technique is often applied to permanently
polarized materials (called electrets when electric, or magnets when magnetic). It
requires a probe that is either conductive or ferromagnetic. The coatings lead to several problems:
Application to more general forces. The nature of the forces sensed by the force gradient technique
can be quite general. The only constraint is that the force be a function of height above surface.
For example, a constant voltage bias between probe and surface produces a vertical force due to
the distance-dependent capacitance between probe and surface (see §3.4, for example).
Material Property Modes
Any mutual force interaction between surface and AFM probe is subject to AFM measurement.
Properties to which the AFM has been applied include:
Many of these are simply special cases of small-amplitude field gradient sensing, as discussed in
§4.
Mechanical properties
When an AFM probe is scanned across a surface, in close proximity, either by closed loop tracking,
or by open loop placement, the interaction forces between probe and surface alter the parameters
of the mechanical resonance of the probe-cantilever system, as discussed in §2.9. Elasticity
alters the resonant frequency ω0, while losses affect primarily Q. Those changes can be detected
through either amplitude or phase modulation of the cantilever motion relative to its exciting
force.
In either case, the average probe Z-axis elevation is usually maintained at some preset value. That
elevation can be maintained in one of two ways:
Force-distance curves. A force/distance (F/D) curve is a measure of the forces on the probe as a
function of distance of the probe from a SUT. It can be measured directly or indirectly.
Direct force-distance curves. A direct force-distance curve is a record of cantilever deflection,
which is proportional to force, while controlling the distance between the probe and the SUT.
Typically a F/D measurement is initiated with the probe in free space, then lowering it until it
interacts with the hard force in the repulsive regime. The probe is then pulled away from the surface
until it is in free space again. This process is illustrated in Figure 3-1.
While the F/D relationship ideally should not depend on the direction of probe motion, in practice
it often does, due to small dissipative (i.e. viscous) forces.
As the probe begins to interact with the surface, it is pulled into the surface by capillary forces.
This process is called jump to contact ( JTC) and often this step breaks the tip off the probe. The
position of the jump to contact is dependent on the thickness of the contamination layer on the
surface. When retracting as the probe is pulled from the surface, the adhesion causes the probe to
"stick" to the surface, and then disengage from the surface.
Errors can occur in the F/D curve if a position sensor is not used to measure the motion in the Z
axis. The error occurs because the Z ceramic generating the motion is not linear and has hysteresis.
It is also necessary to correct the PZT position for the changes in probe position to determine

the actual height of the probe above the surface. Failure to properly correct these errors leads to an
artifact displacement in the F/D curve when the probe is in the repulsive region.
Indirect force-distance curves. Indirect force-distance curves are generated not by measuring cantilever
displacement directly, but rather by measuring the Z-derivative of the force, as discussed in
§2.10. That measurement tends to be less noisy, and thus more accurate, than direct force measurements
because it is carried out in vibrating mode. Numeric integration of the measured dF/dZ can then produce the desired F(Z) curve. Some creativity, of course, is needed in determining the
constant of integration for that calculation (see, for example, Martin et al. (1987). The integration
constant is, in effect, the origin of coordinates - the location of the SUT's "surface".
Indirect F/D curves are subject to most of the same difficulties as the direct F/D curves, other
than the absolute calibration of the Z-axis motion. Its relative linearity is important, but the origin
is determined from the measurements, not the PZT control voltage. Also, if the force is not a
conservative one, that is, if it is not representable as the gradient of a potential energy, then it may
not be a single-valued function of distance.

Pulsed force mode. Pulsed force mode (PFM)
is an "all in one" combination of topography,
adhesion, and stiffness measurements, carried
out simultaneously. PFM is implemented by
placing a sinusoidal voltage on the
Z PZT
and recording the force profile. These properties
can be deduced from key inflection points
in the profile (Figure 3-2).
Surface loading ("nano-indenting"). The resistance
of a surface to normal force distortions
can be measured through the technique that
might be called "nano-indenting." A nanoindent
is generated by forcing the probe into a
surface, causing surface material to be dislodged, creating a
nano-crater. Surface distortion is measured
as a function of normal force. This relationship is called a "loading curve."

Nanoindenting is possible only if the cantilever is stiff enough and
the probe material hard enough. Figure 3-3 shows a nano-crater
created by a silicon probe in a surface of
PMMA.
It is difficult to get quantitative data when nano-indenting with
an AFM because:
Lateral (friction) force mode - nanotribology. As shown in Figure 2-5. the cantilever in an AFM can
twist, or rotate as it is scanned across a surface. Use of the twisting response has opened a new
avenue for the study of friction at the nanoscopic level.
The study of interacting surfaces in relative motion from a macroscopic perspective is known as
tribology, and has been pursued for centuries; its pursuit at the nanoscopic scale has come to be
called nanotribology, and is only a few years old.
It was long thought that there were two fundamental laws of tribology:
While these laws of friction were well-established at the macroscopic level, they prove to be quite
subtle and complex at the small scale accessible to lateral force AFM. The friction force is found
to depend not only on the surface asperity (i.e. gross roughness, as a piece of sandpaper) but also
on intermolecular forces even when the asperity is absent or insignificant. Reitsma et al. explain it
well:
"The fundamental difference between the classical laws of friction and
the laws applying to nanometer scale friction is surface roughness. For
contact between two solid bodies, surface roughness at the interface
means that there are two ways to interpret contact. First is the type that
refers to regions of the interface that are in true (or 'perfect') contact,
often referred to as interfacial contact. The true contact area (At) of an
interface is the sum of all interfacial contacts. The other is the apparent
or gross contact area. This is the macroscopic surface area of the interface
(Ag). Nanotribology attempts to 'scale out' the multiple asperity
contact that describes tribology and the classical laws of friction.
"With reverence to the second classical law of friction (i.e. the proportionality
between friction and load recently both SFA and in particular,
AFM experiments, measuring interfacial friction have demonstrated a
clear non-linear relation between friction and load .."
The frictional coefficient of a probe moving over a surface is defined as the loading force divided
by the horizontal force:

With both vertical and lateral deflections (and thus estimates of the forces) available (see §2.5), it
is possible to determine a friction coefficient. Recalling that the sense of the lateral force is always
in opposition to the scan direction, measurements usually record a curve with hysteresis, as shown
in Figure 3-4. With modest simplifying assumptions, and some dimensional information about
the probe, an effective coefficient of friction may be calculated. Accuracy of the result is often
questionable due to uncertainties in those assumptions.
Figure 3-5 shows lateral force images from a very flat gold test sample. The topography image is
featureless, but the LFM image shows the drawn pattern. It is noteworthy that the appearance of
the pattern is different, depending upon the scan direction.
Thermal modes
Special thermal sensing probes incorporating thermocouples or resistors (Figure 3-6) permit
nano-scale measurement of:
Electrical Modes
Electrical modes involve measurements of localized surface responses to various electric or magnetic
stimuli. Some require direct probe-surface metallic contact and others only near proximity.
Parametric (contact) measurements. By "contact measurements" we mean those that treat the
probe-plus-surface as a two-terminal circuit device. Some sort of V-I characteristic is measured
point-by-point as the probe scans the surface.

Although direct contact is simple in principle, it is difficult
in practice. The interface between probe and surface is
complicated by:
A conductive diamond coat can mitigate issues (b) and (c),
though it increases the diameter of the probe significantly.
The contamination problem is largely independent of
probe material.
Scanning versus static measurements. Although direct contact seems suitable for measuring electrical
properties of nanostructures such as nanotubes or quantum dots, it proves problematic. Positioning
error is a problem. Such structures as nanotubes and quantum dots are extremely small
and difficult to locate. Although smooth scanning at the nanometer scale is easily achievable, it
requires only relative positioning. Absolute, repeatable positioning at that scale, however, is very
difficult.
Ohmic conductivity. Local conductivity of a surface or structures located thereon can be measured
by an AFM. The probe should have high conductivity compared to the SUT, through either its
bulk or through a suitable coating.
Dielectric constant. A conductive probe above a surface, with a constant voltage applied between
them can be considered a simple capacitor. Any capacitor having an adjustable mechanical coordinate, say Z, held at constant voltage, can be shown from energy principles, to exert a force against
that coordinate

where the negative sign signifies the direction that will reduce the capacitance. Our prior analysis
of force gradient sensing (§2.10) remains valid, and equation (2-15) is once again applicable, so
that

SHARK (simultaneous conductivity-topography). In the animal world, the elasmobranchs (the subclass
of cartilaginous fishes that includes skates, rays and sharks), have a unique ability to sense
electric fields (see, for example, Adair et al (1998)). That sense is thought to have played an
important role in their evolution. They use it both for locating prey and for orientation, via
motion-induced sensitivity to the earth's magnetic field. Threshold sensitivity is said to be of the
order of microvolts per meter or less.
SHARK technology®, whimsically named for these remarkable animals, brings similar electric
field sensing to atomic force microscopy. As an acronym it is said to stand for "surface height and
resistivity camera" (if one accepts the German spelling "kamera" .). It is an AFM imaging technique
that produces simultaneous topographic and conductivity maps.
The spatial map of electrical conductivity, as measured with SHARK, once again uses the stimulus-
response apparatus shown in Figure 3-7. The stimulus in this case is constant voltage applied
between the sample and the probe, while the response is current. Measurement of current yields a
conductivity map, while topography is sensed in the conventional contact fashion. The advantage
of SHARK is that the topogram and conductivity map are captured simultaneously during one
scan, reducing test time. Figure 3-9 is a SHARK image of a carbon nanotube held perpendicular
to a conductive substrate.
Contact potential difference (Kelvin probe). Contact potential difference (CPD) is unfortunately
named, as it is something that is invariably measured without contact. It is defined as the potential
difference between dissimilar conductive materials whose mobile electrons are in thermal equilibrium.
It is the difference in work functions of the two materials. That equilibrium leads to small
charge imbalance, and thus a potential difference between the surfaces if they are electrically connected.
Two surfaces, considered as a capacitor, behave as though there were an internal potential
source polarizing the capacitor. That internal potential is equal to the tiny charge difference
divided by the capacitance.
The so-called Kelvin probe method is an age-old technique for measuring CPD. If the two electrically
connected conductors are brought into near proximity, there is a small electric field
between them due to the tiny charge imbalance.


Conventional Kelvin probe measurement places a
fixed voltage across a capacitance formed of the materials to be tested (right). One of the surfaces is
then mechanically vibrated. From elementary circuit
theory one has
The external applied voltage is adjusted until the AC current induced by the vibration is reduced
to zero. The applied is then known to be equal and opposite to the CPD. Readout of that value of
V0 thus provides the desired measurement, after a sign change.

A slight variation on this technique is
eminently well-suited for the AFM,
which adds imaging capability. This
technique is best called Kelvin probe
microscopy (KPM), avoiding the oxymoronic-
seeming "contact potential
difference" that involves no contact.
The AFM version (Figure 3-11)
turns the macroscopic Kelvin probe
method on its head: It applies an AC
voltage to the capacitance formed of
the materials under test, and detects
the resultant vibration. It is easily shown from elementary principles that, for a capacitor whose
capacitance depends on a mechanical coordinate, say, in this case, Z, then there is a force exerted
by the capacitor on its supports:

Using for V the sum of a DC nulling voltage and an AC sense voltage

leads to a component of force at frequency ω that is proportional to V
0, viz:

A major advantage of this technique is that there is no need to calibrate the capacitance or its Z
derivative. It is a nulling method. All that is necessary is to adjust V
0 until the force component at
frequency ω goes to zero. As in a macroscopic Kelvin probe measurement, it is then known that
V0 at null is thus equal to the negative of the CPD. If the nulling process can be carried out sufficiently
rapidly, then recording V0 while raster scanning provides a desired two-dimensional KPM
image.
Several instrumental configurations for KPM are possible. There are two applied stimuli involved:
the cantilever Z-axis mechanical driving force, and the applied voltage. They may be distinguished
by frequency. This permits two-loop configurations in which topography is measured in
conventional fashion, simultaneously with the contact potential map. One such apparatus is
shown in Figure 3-12.

Unlike other imaging methods, scanning
Kelvin probe microscopy is a
quantitative. It measures absolute
potential difference (cf EFM, §3.4,
which measures electric field
strength). Because KPM uses noncontact
VCM to track topography,
there is less tendency to damage the
probe. KPM, however, is more costly
to implement because it requires a
lock-in amplifier and PID controller.
Electric force microscopyElectric force microscopy (EFM) is the examination of surfaces via non-contact electric field
interactions. Primarily this pertains to ferroelectric and piezoelectric materials. Ferroelectric
("electret") materials have a permanent electric polarization. Piezoelectric materials have a dimensional
change in response to applied electric fields, and vice versa. The two properties are often
both present, as the crystal symmetry group requirements are identical. An electret, in effect, is a
piezoelectric material with memory.
The advantage of the AFM probe for ferroelectric measurements is that the probe has high spatial
resolution and localized measurements are possible. There are two primary types of measurements
made on ferro/piezo films: purely electrical properties, and electro-spatial properties.
Electrical responses to electrical stimuli are measured with an apparatus similar to that described
§3.3. The probe is placed in contact with the ferro/piezo film and the electrical measurement is
made.
Dimensional responses to electrical stimuli are measured through cantilever deflection in response
to an applied voltage.
In both cases the response has memory (a.k.a. hysteresis), that is, the result depends on whether
the applied stimulus is increasing or decreasing. Stimulus-response curves have a "butterfly" character,
as illustrated in Figure 3-14, if they are recorded through a full cycle of the stimulus.

The spatial resolution of either type
of measurement is governed primarily
by the probe diameter,though
grain size of Polycrystalline materials
also plays a role.
Magnetic field microscopy
Magnet field microscopy (MFM) is
the examination of surfaces via noncontact
magnetic field interactions.
A probe coated with a ferromagnetic
film is vibrated slightly above a
surface while scanning. Modelling
the magnetization as sparsely distributed
surface dipoles, it can be
shown that the force gradient is
where
s = tip-surface distance
δ= nonmagnetic thickness
R = tip radius
mp = magnetic moment of surface dipole
mt = magnetic moment of probe tip
dm = mean magnetic diameter
and
Though the detailed relationship, derived from (3-11) and (4-5), is somewhat complex, the general
conclusion is that the frequency change is roughly proportional to a moderately high (third to
fifth) power of the separation. It is thus very sensitive to the three-dimensional structure of the
magnetic domains.

AFM in magnetostatic mode is especially useful for examination
of the nanoscale structure of magnetic recording media.
See, for example, Figure 3-15.
As with EFM, the resolution achievable with MFM depends on
the thickness and quality of the probe coating. This is difficult
to control, so that the results from MFM are often inconsistent.
Also, when trying to measure the magnetic domains on a soft
magnetic material, magnetic domains on the probe can alter the
magnetization of the SUT, masking or obliterating the original
properties that were to be measured.
Active Modes
The machinery comprising the AFM can be utilized for active manipulation as well as passive
observation. That is, it can become a toolbox for altering the physical and chemical properties of
the SUT, not just a microscope. The tools in that toolbox include:
Lithography
The term "lithography" originally meant "writing on stone", a technique long-used for printing of
hand-drawn illustrations, as in books and magazines. In modern times it has taken on a connotation
of the creation of micro-structures on semiconductor devices; conventional printing technology
long ago left it behind. The exact definition in the nanoscale context is still in flux, but it
retains its basic meaning of image creation.

Like modern printing, nano-scale AFM
lithography uses one, or the other, or both of
the two basic techniques: bit-mapped imagery
and vector-drawn imagery. As in computer
printers, software renders the desired image
described by a source file (e.g. .bmp or .jpeg).
It moves the probe and indents, scratches, or
deposits "ink" of some kind (Figure 4-1). Resolution
of such AFM lithography, of course,
usually depends upon the probe diameter and
noisiness of the PZT positioning process. The
primary drawback to AFM lithography is low
scan rate.

Simple Scratching. What is a drawback for AFM microscopy can be an asset for surface
etching. If the force exerted by the
probe is high enough, and the SUT is
softer than the probe, the probe will
scratch the surface.
Anodic Oxidation. In 1989 it was demonstrated
that the localized current from a small probe, as
in a scanning tunneling microscope, can modify
a surface through localized electrochemistry.
The most common example is anodic oxidation.
In this particular example, the width of
the oxidized line that is created depends on the
number times it is traced.

Chemical deposition - The AFM as generalized printer/plotter. The AFM can be used as a sort of generalized
plotter, applying a variety of "inks" at the nanometer scale, for a variety of applications.
The vehicle for the deposition can be:
Many applications have been envisioned in which precise deposition or fabrication or lithographic
mask creation at the nano-scale are needed.
The fluid deposited may also be a so-called "molecular glue" which forms a template or mask for
subsequent chemical nano-scale fabrication.
Dip Pen Nanolithography® (DPN
®) is a proprietary scanning probe lithography technique invented
in Dr. Chad Mirkin's laboratory at Northwestern University, in which a microscopic pen (e.g. the
tip of an atomic force microscope cantilever) is coated with an "ink" (a chemical compound or
mixture) and put in contact with the "paper" (a substrate). Both the name and its abbreviation are
now trademarks of the Nanoink corporation. "Dip pen" is an archaic name for a quill pen, by analogy
to the procedure.

Electrochemical experiments
An electrochemical cell can be added to an AFM enabling electrochemistry experiments in situ.
The AFM can then be used to study electrochemical changes in surface properties without thesurface being exposed to air. With the addition of a galvanostat, the surface topography can be
investigated as function of the surface potential relative to a reference cell.
Performance
The AFM is its extremely high effective magnification, several orders of magnitude better than
optical microscopy. Imaging of surface features as small as one atom have been reported (see, for
example, Rugar et al.(2004)). One may, naturally, ask what this really means. Can the "resolution"
be characterized quantitatively? The answer, of course, is yes, but doing so is difficult and complex.
It depends on the specific phenomena being sensed, i.e. on the nature of the probe in use.
Only the most rudimentary AFM applications actually relate to topographic imaging. Most interesting
are applications to various non-visual physical phenomena.
Resolution
Resolution in images is generally taken to mean in-plane (X-Y) resolution. In the AFM one Zaxis
resolution is also of interest. the latter involves both positioning and noise.
X-Y Resolution. Tip effects. One of the most important factors influencing the resolution which
may be achieved with an AFM is the sharpness of the scanning probe. Typical probes have radii of
a few tens of nm; the best tips may have radii less than 10 nm.
The need for sharp tips is normally explained in terms of tip convolution. This is a broad term,
often used incorrectly, to identify several effects on transverse AFM resolution due to the finite
size of the probe tip and the non-ideal interactions between probe and SUT.
The main influences are

Geometrical broadening. Geometrical
broadening arises when the radius of
curvature of the tip is comparable
with, or greater than, the size of the
feature being imaged. Figure 5-1
illustrates this problem. As the tip
scans over the specimen, the sides of
the tip make contact before the apex,
and the microscope begins to respond
to the feature. The effect illustrated
assumes, perhaps naively, that the
probe and the SUT are incompressible. This effect is sometimes called tip convolution.
Tip deconvolution/blind reconstruction. Several researchers have reported methods of partially mitigating
the deleterious effects of the so-called "tip convolution" on image resolution. Particularly
interesting are the techniques denoted "blind reconstruction" or "blind deconvolution," which
require no information about the tip other than the image itself. Villarubbia (1997) describes avariety of algorithms for this in sufficient detail for programming. See Bottomly (1998) for an
extensive bibliography.
Longitudinal compression. Longitudinal compression is distortion caused by z-axis compression of
the SUT by the probe. The importance of this effect is obviously material dependent, and difficult
to quantify. However studies on some soft biological polymers (such as DNA) have shown the
apparent feature widths dependent upon tracking force.
To put this effect in perspective, suppose that a probe has contact area about (10 nm)2, and operates
with a tapping force of 1 nN (both are in the right ballpark). Recalling that 1 N/m2 = 1 pascals,
this is a pressure of about

Smaller probe contact areas and larger forces, of course, yield even larger pressures. Compression
effects on soft samples thus should not be surprising.
Other resolution effects result from the physical nature of the probe-surface interaction. This is
specifically important in vibrating modes when sensing force gradients. The quantitative nature of
the broadening depends on the particular physical phenomenon in question, such as magnetization
mapping, Kelvin probes that make use of fringing fields, surface capacitance, and such.
Z-Axis resolution and noise
Unless one is interested in absolute position, there are only two fundamental source of Z-axis
uncertainty, both of them noise sources:
Although one might expect an effect of the quantized nature of the light being reflected by the
light lever, that proves to be negligibly small.
There are, of course, non-fundamental environmental noise sources, such as man-made, and natural
seismic vibration, ambient noise, airflow. As these are relatively low frequency (10s of Hz at
most), they contribute little to the noisiness of the AFM deflection measurements, which are at
10s of kHz. They do contribute to uncertainty and lack of repeatability in X-Y positioning, tho
this can be mitigated by well-known isolation techniques (very heavy work surfaces on elastomeric
cushions, shock absorbers, draft-blocking enclosures, and the like).
Light lever shot noise. The fundamental limit on noise of the light lever deflection detector is shot
noise in the detector. Moreover, and perhaps surprisingly, diffraction of the sense beam with
increasing "lever" length causes the sensitivity to approach a constant, independent of length once
a critical length is exceeded. The SNR is found to be

where:
λ = wavelength of laser light
η= quantum efficiency of the detector
h= Planck constant
c= speed of light
B= post detection bandwidth
g1= geometrical factor accounting for possible bending of cantilever, ranging
from 0 (fixed cantilever base) to 2 at the maximally moving end.
g2= geometrical factor accounting for cross section of beam =

for a
gaussian beam
D(X) =beam waist diameter as function of distance from its waist
z = displacement of end of cantilever
If the cantilever is assumed to move as a rigid body (not an unreasonable approximation), then
g1
= 1, and the beam deflection is 2Δz/λ, the factor of two accounting for the fact that the beam
angle doubles the mechanical angle upon reflection.
The beam diameter as a function of distance is

This is a consequence of the hermite-gaussian beam structure that exits the confocal laser resonaters
(see, for example, Boyd et al. (1961 and 1962), or Kogelnick and Li (1966)). The asymptotic
SNR in the far field of the gaussian beam (where D is growing linearly with distance) is
found from (5-2) and (5-3) to be
independent of X. The detector, of course, must be large enough in diameter to intercept substantially
all of the beam at the distance used.
That threshold far-field distance is defined by the second term of (5-3), that is

For a rough idea of that distance, suppose D0 ≈ 1 mm and λ = 780 nm. Then (5-5) gives the minimum
distance as X > 4 m.
For distances smaller than (5-5), where the beam diameter is sensibly constant, the SNR does
grow with X, as naive intuition would lead one to expect.
Putnam et al (1992) compare the sensitivity of several variations on the light lever, as shown in the
table below. The parameters chosen for the theoretical analyses are reasonable practical values.
Note that, for a post detection bandwidth of 10 kHz, the values of ΔZmin in the table range from
about 0.008 Å to 3 Å. The high end of this range is only a few hydrogen atom diameters; even the
poorest of implementations is remarkably sensitive.
Note further, that Putnam et al. also show that the performance of the light lever technique is
comparable (i.e. within a factor of two or so) of that the interferometric technique, with comparable
detectors. As the interferometers tend to be more complex (read: expensive), the light lever
generally is to be preferred.

Light lever thermal noise. Perhaps surprisingly, the most serious limitation on AFM Z-axis performance
is thermal vibrations of the cantilever itself. As is well known from elementary statistical
mechanics, the equipartition theorem says that every degree of freedom of a electrical or mechanical
system at absolute temperature T has average energy KT, where KB is Boltzmann's constant ≈
1.38*10-23 joules per kelvin. In the case of the elementary mass-spring oscillator embodied in the
simple probe-cantilever model that energy is equally divided between kinetic and potential. Thus
the average kinetic energy is
Assuming that motion is approximately sinusoidal with random amplitude and phase, one finds
easily from (5-6) and the fact that the average square of any sinusoid is ½, that
For typical values of this thermal noise level, one can consult the catalog of, for example,
Nanosensors™, whose advertised values of k lead to the rms thermal noise amplitudes shown in
Table 4:. These noise levels are larger by orders of magnitude than the light lever shot noise discussed
discussed
above, and are thus the primary limitation on AFM Z-axis resolution. Their deleterious
effect, however, can be partially mitigated through the used of vibrating mode techniques, which
can use narrow post-detection bandwidths. The noise shown in the table has the spectrum of the
cantilever resonance, whose bandwidth is f0/Q, typically a few hundred Hz.
Other considerations
The above resolution and noise considerations are the primary limitations on AFM performance,
there are other potential issues that sometimes arise:
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