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.

Picturing Earth in a new light

Maps can show more than just where things are—they can also show how things change. New maps of artificial light reveal a planet that has been reshaping its nights through patterns of brightening and dimming.

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 ...

page 1 from 8