What are the steps involved in AFM probe calibration

Mar 16, 2026

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The core steps of AFM probe calibration include environmental preparation, probe installation, laser alignment, Z-axis and XY-axis calibration using standard samples, and system error control. The entire process must strictly adhere to operational protocols to ensure the accuracy of nanoscale measurements.

 

I. Pre-Calibration Preparation: Environmental Control and Equipment Initialization

Atomic Force Microscopes (AFM) are extremely sensitive to their environment; therefore, it is essential to ensure the system is in a stable state prior to calibration:

Environmental Control: Maintain the laboratory temperature between 20–25°C and humidity between 40%–60% to prevent thermal expansion and changes in surface adsorption layers from affecting measurements.

Vibration Isolation: Place the instrument on a dedicated vibration-isolation platform, situated away from vibration sources such as high-frequency equipment or air conditioning vents.

Power Grounding: Ensure the power supply utilizes single-point grounding to prevent electromagnetic interference from increasing signal noise.

Power-on Warm-up: Switch on the AFM main unit and controller, allowing them to warm up for at least 30 minutes to ensure the piezoelectric ceramics and electronic components reach thermal equilibrium.

Key Tip: Environmental fluctuation is one of the primary sources of system error; a temperature variation exceeding 1°C can induce significant thermal drift.

 

II. Probe Installation and Optical System Alignment

1. Probe Selection and Installation

Select the appropriate probe based on the experimental mode (Contact, Tapping, or Non-contact):

For Tapping mode, probes with a high resonance frequency and low spring constant (e.g., 300 kHz, 40 N/m) are recommended.

For hard samples, diamond-coated probes may be selected to extend probe lifespan.

During installation, use tweezers to gently grasp the probe holder; avoid touching the cantilever or the tip itself to prevent mechanical damage.

2. Laser Alignment

Switch on the laser and adjust the position of the emitter so that the laser spot is precisely focused on the rear section of the cantilever's reflective area.

Adjust the position of the detector (a four-quadrant photodiode) to ensure the signal intensity reaches at least 80% of the full scale, thereby guaranteeing sensitive force feedback.

If utilizing the "ScanAsyst" intelligent mode, the system can automatically optimize the amplitude setpoint, thereby minimizing human error.

Verification Criteria: By observing the force curve test, verify that the baseline is stable and free of sudden jumps, thereby confirming that the laser alignment is correct.

 

III. Calibration of Core Parameters Using Standard Samples

1. Z-Axis Sensitivity Calibration (Vertical Calibration)

Standard Sample: Select a Si(111) crystal plane atomic step (theoretical height: 0.19 nm) or a TGZ-series Z-direction standard (e.g., TGZ1: 20.0 ± 1.5 nm).

Procedure:

Scan the standard step region to acquire a height profile.

Calculate the ratio of the measured height to the theoretical value, and adjust the gain parameter of the Z-axis piezoelectric transducer accordingly.

Repeat measurements on multiple steps to obtain an average value, thereby enhancing calibration accuracy.

Error Compensation: Employ a dual-step standard covering 10%–70% of the instrument's full measurement range; use the area-averaging method to correct for Z-axis displacement nonlinearities.

2. XY-Axis Scanner Calibration (Lateral Calibration)

Standard Sample: Use a TGG1 X/Y-direction calibration standard (periodicity: 3 ± 0.05 µm) or a TGX1 checkerboard-patterned square pillar array (height: ~0.6 µm).

Procedure:

Scan a large area at low magnification to check for image distortion or angular misalignment.

Measure the actual scanned distance of a structure with a known periodicity to calculate the pixel dimensions (nm/pixel) in the X and Y directions.

Input the correction factors into the software to eliminate scanner nonlinearities and cross-coupling effects.

3. Probe Tip Shape Assessment (Tip Characterization)

Standard Sample: Use a TGT1 3D tip calibration standard or an SHS-series step standard (pyramidal structure: 50–100 nm).

Objective: Assess whether the probe tip has become blunted or contaminated, thereby preventing "tip convolution" effects that lead to image broadening.

Method: Reconstruct the tip profile by analyzing the acquired image, and apply deconvolution algorithms to correct for the true topography of the actual sample.

 

IV. System Error Control and Maintenance Strategies

1. Analysis of Major Error Sources

Error Type

Source

Control Method

Scanner Nonlinearity

Piezoelectric hysteresis, creep

Periodically calibrate using standard samples; avoid prolonged continuous scanning.

Detector Noise

Laser fluctuations, circuit interference

Keep the optical path clean; maintain signal strength > 80% and RMS noise < 0.1 nm.

Probe Drift

Temperature fluctuations, mechanical relaxation

Warm up the instrument for 30 minutes prior to experiments; enable drift compensation algorithms during scanning.

Tip Convolution

Tip dulling or contamination

Periodically check tip condition using a TipCheck sample; replace the tip promptly.

2. Standardized Maintenance Procedures

After Each Use

Clean the sample stage with an ethanol-soaked cotton swab to prevent dust accumulation.

Weekly Check

Use a TipCheck sample (containing 4.5 nm particles) to assess probe sharpness.

Annual Recalibration

Have a professional institution perform metrological recalibration, focusing on verifying Z-axis repeatability (standard deviation should be < 1 nm).

3. Adherence to International Standards

ISO 11039

Specifies definitions and calibration procedures for SPM dimensional measurements.

ASTM E2530

Covers guidelines for AFM laboratory practices.

GB/T 31227-2014

Chinese National Standard; standardizes methods for nanoscale length measurements.

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