Key takeaways
- HD-KFM™ III, single-pass KPFM on the Nano-Observer II, resolves grain-boundary potential contrast in perovskite thin films at sub-10 nm resolution.
- Illuminated KPFM (surface photovoltage) compares dark and illuminated conditions on the same area.
- ResiScope™ III maps grain-level conductivity in perovskite films and doped-layer interfaces in silicon solar cells, over several orders of magnitude in one pass.
- Soft ResiScope™ separates conductive P3HT and insulating PMMA domains in organic solar-cell blends without damaging the film.
Animated story
The same question, at the nanoscale
What a solar cell does under light depends on how the light arrives. Reproduce the angle, and you reproduce the condition — then measure the response where it happens, on the surface.
01
The same range the sun covers over a day
Irradiance follows the elevation, from 20° to 90°.
02
Reproduce the angle
…and you reproduce the condition the cell sees in the field.
03
The same sweep, on the microscope
Continuously adjustable on a graduated arc, locked at any angle onto the sample.
Measurement check
A known potential, measured

Before interpreting potential contrast on an unknown film, KPFM can be checked on a structure whose potential is set externally. With the electrodes biased, the HD-KFM map shows the applied potential as a uniform level on each electrode and how it spreads into the surrounding surface. The same HD-KFM image is shown on the HD-KFM™ III page with other reference samples.
Summary
Conclusion
HD-KFM™ III maps grain-boundary surface potential in perovskite thin films in a single pass, and repeating the scan on the same area under illumination gives the surface photovoltage. ResiScope™ III adds grain-level conductivity in perovskite films and the doped-layer interfaces of silicon cells over several orders of magnitude in one scan, while Soft ResiScope™ separates conductive and insulating domains in organic blends without damaging the film. Acquired on the same Nano-Observer II and correlated in NanoSolution, these channels link the nanoscale structure of a photovoltaic film to the potential and current that govern device performance.
Published work
Research published with CSInstruments AFMs
Peer-reviewed studies on perovskite, photoresponsive and solar-fuel materials in which CSInstruments AFMs were used. More on the publications page.
- M. Vila, J. Bartolomé, A. El Astal-Quirós, et al. Morphology engineering of MAPbBr3 thin films for enhanced lighting applications. APL Mater. 2025, 13 (7): 071109.
- M. Maniadi, K. Tieriekhov, O. Ségut, et al. From the Bulk to the Nanoscale: Strong Evolution in the Structure and Chiroptical Properties of Chiral Halide Double Perovskites. Adv. Optical Mater. 2025, 13, 2402949.
- V. Virole, N. Dabke, S. Verma, et al. Visible range photoresponse of an organic single-crystal analogue of green fluorescent protein. Nanoscale 2025, 17(14), 8614-8623.
- V. Guigoz, S. Bruyère, T. Gries, et al. Copper substitution in lanthanum-deficient LaFeO3 for enhanced solar hydrogen production. Int. J. Hydrogen Energy 2025, 148, 150072.
In this application note
AFM scans and modes in this note
- AFM scan of perovskite thin film — HD-KFM™ III surface potential: potential contrast at grain boundaries, resolved in a single pass.
- AFM scan of perovskite solar cell film — ResiScope™ resistance: resistive grain boundaries and conductive grain interiors.
- AFM scan of silicon solar cell cross-section — ResiScope™ resistance: doped layer interfaces and resistance gradients.
- AFM scan of P3HT/PMMA organic solar cell blend — Soft ResiScope™: phase-separated conductive and insulating domains, no mechanical damage.
AFM modes used
FAQ
Frequently Asked Questions
Why use KPFM for perovskite solar cell characterization?
KPFM (Kelvin Probe Force Microscopy) is the primary technique for mapping nanoscale surface potential and built-in electric fields in perovskite solar cells. It reveals grain boundary potential variations (typically 50–200 mV higher than grain interiors), local open-circuit voltage (Voc) distribution, charge trap density, and band bending at ETL/perovskite and HTL/perovskite interfaces. These measurements directly correlate with device efficiency losses and degradation mechanisms that are invisible to macroscopic characterization techniques.
What does KPFM show at grain boundaries in perovskite films?
KPFM surface potential maps of perovskite films consistently show that grain boundaries exhibit distinct potential contrast compared to grain interiors. Depending on composition and processing, grain boundaries can show positive or negative potential shifts of 50–300 mV. These variations indicate local work function differences caused by ion accumulation, defect states, or compositional segregation at grain boundaries. HD-KFM III single-pass mode on the Nano-Observer II resolves these boundary features at sub-10 nm resolution, enabling correlation with grain size, orientation, and processing conditions.
How does ResiScope AFM characterize perovskite solar cells?
ResiScope™ maps local current and resistance across the perovskite film surface at nanoscale resolution. Its 10-decade dynamic range (fA to μA, 10² to 10¹² ohms) in a single scan pass allows simultaneous visualization of both highly conductive grain cores and highly resistive grain boundaries or insulating domains — without manual gain adjustment. This is critical for perovskite because resistance variations of several orders of magnitude exist within a single 2–10 µm scan area. ResiScope measurements identify current-blocking grain boundaries, shunting pathways, and local conductivity heterogeneity that directly affect photovoltaic performance.
What AFM is best for perovskite solar cell research?
The Nano-Observer II by CSInstruments is purpose-suited for perovskite AFM research. It combines HD-KFM III (single-pass surface potential with sub-10 nm resolution) and ResiScope III (10-decade electrical mapping) in one system. Critical for perovskite work: glove-box compatibility for air-sensitive samples, optical coupling for illuminated KPFM (light-on/light-off experiments), electrochemical cell option for in-situ ionic transport studies, and temperature stage (-40°C to 450°C) for stability testing. The AutoScan software with automated approach and gain control reduces operator-induced artifacts on these sensitive films.
Can KPFM measure illuminated perovskite solar cells?
Yes. The Nano-Observer II has an open optical design that allows light illumination during KPFM measurements. Illuminated KPFM (also called surface photovoltage mapping) compares surface potential maps acquired in dark and under controlled illumination, directly revealing photogenerated carrier separation, local quasi-Fermi level splitting, and regions of charge recombination. These experiments are essential for understanding how grain boundaries act as either charge recombination centers or charge transport highways under operating conditions.
Can perovskite films be measured without exposure to air?
Yes. The recommended protocol starts with sample preparation in a glove box, and the Nano-Observer II can operate inside a glove box, so moisture- and oxygen-sensitive perovskite films are measured without exposure to air.
How are organic solar cells measured without damaging the film?
With Soft ResiScope, friction-free resistance mapping in intermittent contact. On a P3HT/PMMA blend it resolves the conductive P3HT and insulating PMMA domains without mechanical damage to the organic film.
What is the recommended AFM protocol for perovskite solar cells?
Prepare the sample in a glove box, survey the topography in resonant mode, measure the surface potential in the dark with HD-KFM III, repeat under illumination for the surface photovoltage, map resistance and current with ResiScope III, then correlate the channels in the NanoSolution software.