Page 5: Research news on aurora

Aurora is a geomagnetic and atmospheric optical phenomenon arising from the interaction of charged particles, primarily electrons and protons from the solar wind and magnetospheric plasma, with atoms and molecules in a planet’s upper atmosphere. Guided by magnetic field lines into high-latitude auroral ovals, these particles precipitate and undergo collisional excitation and ionization of atmospheric species such as oxygen and nitrogen. Subsequent radiative de-excitation produces characteristic emissions, notably green and red lines of atomic oxygen and molecular nitrogen bands, forming dynamic structures including arcs, curtains, and patches whose morphology and intensity are modulated by magnetospheric dynamics and space weather conditions.

NASA's PUNCH mission to revolutionize our view of solar wind

The Earth is immersed in material streaming from the sun. This stream, called the solar wind, is washing over our planet, causing breathtaking auroras, impacting satellites and astronauts in space, and even affecting ground-based ...

NASA CubeSat finds new radiation belts after May 2024 solar storm

The largest solar storm in two decades hit Earth in May 2024. For several days, wave after wave of high-energy charged particles from the sun rocked the planet. Brilliant auroras engulfed the skies, and some GPS communications ...

Lightning strikes link weather on Earth and weather in space

There are trillions of charged particles—protons and electrons, the basic building blocks of matter—whizzing around above your head at any given time. These high-energy particles, which can travel at close to the speed of ...

NASA rockets to fly through flickering, vanishing auroras

Two NASA rocket missions are taking to the Alaskan skies in hopes of discovering why some auroras flicker, others pulsate, and still others are riddled with holes. Understanding these peculiar features is part of NASA's goal ...

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