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Super-Resolution of SOHO/MDI Magnetograms of Solar Active Regions Using SDO/HMI Data and an Attention-Aided Convolutional Neural Network
DOI: 10.1007/s11207-024-02283-1 Bibcode: 2024SoPh..299...36X

Xu, Yan; Wang, Haimin; Wang, Jason T. L. +4 more

Image super-resolution is an important subject in image processing and recognition. Here, we present an attention-aided convolutional neural network for solar image super-resolution. Our method, named SolarCNN, aims to enhance the quality of line-of-sight (LOS) magnetograms of solar active regions (ARs) collected by the Michelson Doppler Imager (M…

2024 Solar Physics
Hinode SOHO 4
Improving the Spectral Resolution and Wavelength Scale of SDO/EVE MEGS-A Flare Observations
DOI: 10.1007/s11207-024-02394-9 Bibcode: 2024SoPh..299..151G

Chamberlin, Phillip; Gonzalez, Gabriela; Herde, Vicki

The Extreme ultraviolet Variability Experiment (EVE) is one of three instruments onboard the Solar Dynamics Observatory (SDO). This paper focuses on using the "A" channel on the Multiple EUV Grating Spectrographs (MEGS-A) on EVE, which measures wavelengths of 5 – 37 nm, to improve the wavelength scale accuracy and spectral resolution during solar …

2024 Solar Physics
Hinode 0
Solar Soft X-ray Irradiance Variability III: Magnetic Field Variations of Coronal X-ray Features
DOI: 10.1007/s11207-024-02289-9 Bibcode: 2024SoPh..299...46K

Matsumoto, Takuma; Masuda, Satoshi; DeLuca, Edward +7 more

The magnetic field changes the radiative output of the Sun and is the main source for all the solar surface features. To study the role of the underlying photospheric magnetic field in relation to emission features observed in the solar corona, we have used the full-disk soft X-ray images from Hinode/X-Ray Telescope (Hinode/XRT) and the magnetogra…

2024 Solar Physics
Hinode 0