Page 3: 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 probe data suggests a more complex sun's magnetic engine

A Southwest Research Institute-led study found that protons and heavy ions react differently to solar magnetic reconnection events, revealing a more complex magnetic engine powering the solar wind. Magnetic reconnection converts ...

JWST reveals surprising secrets in Jupiter's northern lights

An international team of scientists, led by a Ph.D. researcher from Northumbria University, has made further discoveries about a spectacular feature of Jupiter's northern lights, revealing a never-before-seen temperature ...

Auroras on Ganymede and Earth share striking similarities

New observations of Ganymede reveal a striking similarity between the auroras on the largest moon in the solar system and those on Earth. The international team of astrophysicists, led by researchers from the University of ...

Webb maps the mysterious upper atmosphere of Uranus

For the first time, an international team of astronomers have mapped the vertical structure of Uranus's upper atmosphere, uncovering how temperature and charged particles vary with height across the planet. Using Webb's NIRSpec ...

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