Miloslav Druckmüller and his team conduct research during total solar eclipses, utilizing specialized equipment to observe the sun's outer atmosphere, the corona. This work involves setting up portable telescopes and cameras connected to laptops in locations within the path of totality, such as the plains of Castile and León in Spain.
Druckmüller designed and built a unique optical instrument comprising eight astrocameras. Each camera is fitted with a spectral filter designed to detect and record specific emission spectra originating from the solar corona. These spectra are linked to particular ionic species of iron atoms.
The temperature required to ionize iron varies depending on the specific ionic species. By analyzing the locations and relative abundance of these different iron ionic species, researchers can gain insights into the distribution of heat within the solar corona. This method aims to address long-standing questions about the sun's outer atmosphere.
Druckmüller has spent decades developing the custom-built telescope systems and image-processing techniques used in this research. His experience includes observing 19 solar eclipses, demonstrating a long-term commitment to this specialized field of solar physics.
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Miloslav Druckmüller leads a research team using custom-built optical instruments and image-processing techniques to study the solar corona during total solar eclipses. Their goal is to map the temperature distribution within the corona by analyzing specific emission spectra from iron ions, which helps solve long-standing solar mysteries.