• Magnetic waves behind decades-long mystery of solar wind acceleration

    A team of scientists compared data from NASA’s Parker Solar Probe and ESA’s Solar Orbiter and discovered that magnetic waves known as Alfvén waves, essentially a form of plasma wave, are responsible for pumping energy into the solar wind, causing it to accelerate and heat up as it travels away from the Sun.

  • Origins of solar wind revealed

    The origins of the constant flow of charged particles from the Sun, known as the solar wind, and the details of the transition from defined rays in the Sun's upper atmosphere to the solar wind have been a mystery ever since the discovery of solar wind in 1950s….

  • Solar wind stream buffers Earth magnetic field

    Earth is currently inside a solar wind stream flowing in from the massive coronal hole on the Sun's northern hemisphere. Elevated solar wind speed (above 600 km/s) combined with a south tilting Bz component of Interplanetary magnetic field (IMF) is responsible

  • Geomagnetic storm still in progress (June 2, 2013)

    The arrival of an interplanetary shock wave on May 31, 2013 caused geomagnetic storming that reached G2 (Moderate) geomagnetic storm levels on NOAA/SWPC storm scale during June 1, 2013. The solar wind speed remains elevated above 650 km/s. Currently, geomagnetic

  • Intro to space weather vocabulary – video

    Heliophysics scientists study energy transformation from one event to the other and which electromagnetic waves create which conditions near Earth. Space weather effects can disrupt satellites in space, so scientists need to understand the system in even more detail.

  • New research to focus on energy distribution in upper atmosphere

    “Understanding interaction between the Earth’s magnetic field, or magnetosphere, and its upper atmosphere – known as the thermosphere/ionosphere – is especially important this year and in 2014, said Yue Deng, an assistant physics professor at University of Texas.

  • Researchers discovered source of solar wind energy

    Researchers have found signs of an energy source in the solar wind, a hot and fast flow of magnetized gas that streams away from the sun’s upper atmosphere. Solar wind is made of hydrogen and helium ions with a sprinkling of heavier elements. Solar wind is

  • Zooming in on charged particles emitted by the Sun

    Using ESA’s Cluster satellites as a space plasma microscope, scientists have zoomed in on the solar wind to reveal the finest detail yet, finding tiny turbulent swirls that could play a big role in heating it.Turbulence is highly complex and all around us, evident