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Ultraviolet–visible (UV–visible or UV–Vis) spectroscopy is an analytical technique that investigates the interaction between matter and UV–Vis light within the electromagnetic spectrum. This method is widely used for its versatility, simplicity, and relatively quick data acquisition, making it valuable for both qualitative and quantitative analysis. When UV–Vis radiation passes through a material,  molecules absorb light depending on the energy required for...
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UV–Visible absorption spectra of conjugated dienes arise from the lowest energy π → π* transitions. The light-absorbing part of the molecule is called the chromophore, and the substituents directly attached to the chromophore are called auxochromes. A strong correlation exists between the absorption maxima, λmax, and the structure of a conjugated π system. The Woodward–Fieser rules predict the value of λmax for a given structure by adding the...
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The absorbance of UV and visible (UV–visible) radiations is measured using a UV–visible spectrophotometer. Deuterium lamps, which emit UV radiation, and tungsten lamps, which produce radiation in the visible region, are used as light sources in UV–visible spectrophotometers. A monochromator or prism is used for diffraction grating, i.e., to split the incoming radiation into different wavelengths. A system of slits is used to focus the desired wavelength on the sample cell.
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Attenuated total reflectance (ATR) infrared spectroscopy is a powerful analytical technique used to study the composition of materials. It is widely employed in chemistry, materials science, forensic science, and other fields where sample characterization is required. ATR has several advantages over traditional transmission IR spectroscopy, including the requirement of little to no sample preparation and the ability to analyze a wide range of samples.
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When light passes through a substance, a portion of the light is absorbed while the remaining light is reflected or transmitted. If the molecule absorbs light between the wavelengths of 180–400 nm range, the UV spectrum is obtained, and if it absorbs light in the 400–780 nm wavelength range, the visible spectrum is obtained.     
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Quality Assessment of Solar EUV Remote Sensing Images Using Multi-Feature Fusion.

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Summary
This summary is machine-generated.

This study presents a hybrid AI framework for assessing solar Extreme Ultraviolet (EUV) image quality. Combining deep learning and physical indicators achieves high accuracy in automated quality control for space science.

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Area of Science:

  • Space Science
  • Solar Physics
  • Remote Sensing

Background:

  • Accurate quality assessment of solar Extreme Ultraviolet (EUV) imagery is crucial for reliable space science data and weather forecasting.
  • Existing methods may lack robustness in identifying subtle image degradations.

Purpose of the Study:

  • To develop a robust hybrid framework for automated quality assessment of solar EUV remote sensing imagery.
  • To enhance the reliability and accuracy of solar EUV data analysis pipelines.

Main Methods:

  • A hybrid framework fusing deep semantic features (HyperNet-based) with 22 handcrafted physical/statistical quality indicators was developed.
  • A 24-dimensional feature vector was created by combining these diverse feature types.
  • A dataset of 47,950 degraded images simulating seven degradation types was generated from high-quality solar EUV images.

Main Results:

  • An XGBoost classifier trained on the fused features achieved 97.91% accuracy and an Area Under the Curve (AUC) of 0.9992.
  • The hybrid approach demonstrated superior performance compared to methods using only one type of feature.
  • The framework proved robust in classifying image quality across various simulated degradations.

Conclusions:

  • Combining deep learning features with handcrafted indicators significantly improves the robustness of solar EUV image quality classification.
  • This hybrid approach offers a scalable and effective solution for automated quality control in solar observation data processing.
  • The developed framework contributes to enhanced data reliability for space science applications and space weather forecasting.