Observation and modeling of small spatial structures of solar radio noise storms using the UGMRT by S. Mondal et al. – European astronomer radio community

One of the most commonly observed solar radio sources in metric and decametric wavelengths are the so -called solar noise storms. These are generally associated with active regions and are believed to be driven by the plasma emission mechanism. Since plasma emission emits mainly in the fundamental and harmonic of the frequency of local plasma,…

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2025: The Year to Talk About Outcome-based Learning

In the evolving landscape of professional development, the year 2025 marks a pivotal moment as we delve into the significance and purpose of outcome-based upskilling.   Traditional training models are undergoing a transformation, emphasizing the need for a more dynamic and responsive approach that focuses on measurable results and real-world applications. This discussion aims to unravel…

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