A new study led by the University of Hawaiʻi at Mānoa has refined scientists’ understanding of the amount of hydrogen, helium and other elements present in violent outbursts from the Sun, and other types of solar “wind,” a stream of ionized atoms ejected from the Sun.Coronal mass ejections (CME) are giant plasma bursts that erupt from the Sun, heading into the solar system at speeds of 2 million miles per hour. The majority of CME atoms are hydrogen. When the particles interact with Earth’s atmo... ASTRO WATCH · 2 months
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Solar system acquired current configuration not long after its formation  PHYS.ORG · 2 weeks
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New carbon dot-based method for increasing the efficiency of solar cells and LEDs  PHYS.ORG · 2 weeks
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X-rays reveal in situ crystal growth of lead-free perovskite solar panel materials  SCIENCE DAILY · 2 days
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Density fluctuations in the solar wind based on type III radio bursts  PHYS.ORG · 1 week
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Efficient, stable silicon tandem cells enabled by anion-engineered wide-bandgap perovskites  Science Magazine · 2 weeks
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