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MFPN-ASPP: MobileNet Feature Pyramid with ASPP for Photovoltaic Panel Defect Segmentation

MFPN-ASPP pairs a MobileNetV2 encoder, an FPN decoder and an ASPP head to produce pixel-level masks of defects in drone thermal images of solar panels. Here is how it works, what its reported results mean, and where the evidence stops.
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MFPN-ASPP is a segmentation network for photovoltaic (PV) thermal images. It takes a thermal image of a solar installation and outputs a pixel-level binary mask that marks anomalous regions. In the Scientific Reports paper by Galal et al., published 8 October 2026, the authors report a Dice score of 0.8440 and an IoU of 0.7564 on a single dataset of 1,009 drone-captured thermal images from one solar plant in South Africa. These are measurements on that benchmark, not a guarantee of how the model will perform at another site.

What the name means

The title names four pieces. The task is defect segmentation: instead of labeling a whole panel image as faulty or healthy, the model assigns every pixel to either anomaly or background, which is what binary semantic segmentation means. MobileNet (here MobileNetV2) is the lightweight convolutional encoder that extracts features from the image. Feature pyramid refers to a Feature Pyramid Network (FPN) decoder that merges features taken at several depths of the network, so that both small and large anomalous regions are represented. ASPP, atrous spatial pyramid pooling, is a head that processes the merged features at several receptive field sizes to add surrounding context.

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How the model turns a thermal image into a mask

  1. Normalize the thermal image. The paper’s processing flow starts by normalizing the input thermal image before feature extraction.
  2. Extract features with MobileNetV2. The encoder produces feature maps at several scales.
  3. Fuse the scales with FPN. The decoder combines those maps into one multi-scale representation.
  4. Add context with ASPP. The fused representation passes through the ASPP head.
  5. Output probabilities and a mask. The model produces a defect probability for every pixel. A probability threshold of 0.5 converts these into the final binary mask.

Inside the ASPP head

The ASPP head runs four parallel branches over the fused features:

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  • Three convolution branches with dilation rates 1, 6 and 12. A dilation rate spaces the filter taps further apart, so a filter sees a wider area without adding parameters. A rate of 1 is an ordinary convolution.
  • A global average pooling branch, which summarizes the whole feature map into one context vector.

The branch outputs are concatenated and projected, and only then upsampled to the output resolution.

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The thermal dataset behind the results

The paper evaluates on a dataset it credits to Pierdicca et al. as the Photovoltaic Thermal Images dataset. The table lists what the paper says about it.

Attribute As described in the paper
Images 1,009, each at 512 × 640 resolution
Labels One expert-annotated binary mask per image
Site 66 MW ground-mounted facility in Tombourke, South Africa
Capture window 21–27 January 2019
Conditions Clear skies, high irradiance
Sensor UAV-mounted radiometric thermal camera; make and model not named
Recorded thermal values 2.25 to 103.34 °C

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Training and evaluation setup

  • Optimizer and schedule: Adam, learning rate 1 × 10⁻⁴, batch size 4, trained for 200 epochs.
  • Loss: an equal 0.5/0.5 combination of binary cross-entropy with logits and Dice loss.
  • Augmentation: horizontal flips, brightness and contrast changes, and shift, scale and rotation transforms.
  • Validation and testing: run without augmentation.
  • Stability: the paper reports five repeated training runs for stability analysis.

Reported results

Every figure in this section is the authors’ measurement on this dataset and protocol. The abstract summarizes the outcome in one sentence: “The results highlight the efficacy of lightweight encoder–decoder frameworks that incorporate atrous spatial pyramid pooling, enabling accurate and computationally efficient fault detection in photovoltaic installations.” That is the paper’s own statement, not a quotation from a named author.

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Headline metrics

Metric MFPN-ASPP What it measures
Dice 0.8440 Overlap between predicted and annotated anomaly pixels
IoU 0.7564 Intersection over union of predicted and annotated anomaly pixels; usually reads lower than Dice for the same prediction
Precision 0.8771 Share of predicted anomaly pixels that are annotated anomalies
Recall 0.8428 Share of annotated anomaly pixels the model flags
Boundary F-score (2-pixel tolerance) 0.8436 Agreement between predicted and annotated edges, counting an edge as matched if it falls within 2 pixels

Test-set results

In its per-image results, the paper reports a 101-image test set with mean Dice 0.844 ± 0.165 and mean IoU 0.757 ± 0.187. The ± values are as printed in the paper. Per-image scores vary considerably around these means, so an individual image can score well above or below the average.

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What the ablation shows

Configuration Dice IoU
MobileNetV2-FPN (no ASPP) 0.6872 0.5234
MobileNetV2-FPN + ASPP (MFPN-ASPP) 0.8440 0.7564

The gap between these two rows is the gain the paper attributes to adding ASPP, measured on the same dataset.

Comparison with other architectures

The paper reports that MFPN-ASPP scores higher than U-Net, LinkNet, FPN and Mask-RCNN on Dice and IoU. The individual baseline values are in the paper’s comparison results, and they should be read alongside the same training and evaluation protocol the authors used for MFPN-ASPP. These are within-paper comparisons, not a ranking of these architectures across datasets or implementations.

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Efficiency and drone inspection: what is claimed and what is shown

The authors describe MFPN-ASPP as computationally efficient and suitable for UAV inspection. That is their interpretation of a benchmark experiment, not a field trial. The paper does not provide a validated hardware benchmark that supports a specific real-time speed or energy figure for a given drone or onboard computer, so the suitability claim should be read as the authors’ view.

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How to read the metrics for PV inspection

  • False alarms. A precision of 0.8771 means that roughly 12% of predicted anomaly pixels fall outside the annotated anomalies. In a maintenance workflow, those are healthy areas that would still cost a site visit or a closer look.
  • Missed anomalies. A recall of 0.8428 means that roughly 16% of annotated anomaly pixels are not flagged. Those are defects the model would leave unreported.
  • Area versus edges. Dice and IoU reward overlapping area. The boundary F-score asks whether predicted edges land close to annotated ones. A 2-pixel tolerance corresponds to a different physical distance on each flight, depending on altitude and sensor resolution.
  • Masks, not panel verdicts. These metrics score agreement between masks. They do not, by themselves, establish whether each panel is correctly classified as faulty or healthy.

Getting the data and code

  1. Open the article page and go to its data availability statement.
  2. Submit the dataset request form that the statement describes, giving your research purpose. Access is granted on that basis; the dataset is not presented as an unrestricted public download.
  3. For the code, contact the corresponding author named on the article. The paper says code is available upon request.
  4. Check the statement again before you rely on it, because access arrangements can change after publication.

Using the result responsibly

  • When comparing with another segmentation model, use the same image set, annotation masks and train/test split, with matching preprocessing, loss, augmentation and metric definitions.
  • Use the same 0.5 probability threshold when converting outputs to masks, or report the threshold you used.
  • Test the model on imagery from your own sites, sensors and flight conditions before relying on it. The paper’s results do not transfer automatically to other installations.
  • If you plan to acquire imagery, verify radiometric capability, UAV compatibility and current availability for any camera independently. The paper names no make or model, so it does not establish that a particular camera will reproduce its imagery.

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