Page 6: Research news on space weather

Space weather refers to the time-varying conditions in near-Earth space and throughout the heliosphere driven primarily by solar activity, including the solar wind, coronal mass ejections (CMEs), solar flares, and variations in the interplanetary magnetic field. As a physical phenomenon, it encompasses the coupling of solar outputs with Earth’s magnetosphere, ionosphere, and thermosphere, producing geomagnetic storms, substorms, ionospheric disturbances, and energetic particle events. These processes are governed by magnetohydrodynamic and plasma-physical interactions, including magnetic reconnection, wave–particle interactions, and particle acceleration, and are quantitatively characterized using indices such as Kp, Dst, AE, and measures of solar wind and IMF parameters.

NASA's CODEX captures unique views of sun's outer atmosphere

Scientists analyzing data from NASA's CODEX (Coronal Diagnostic Experiment) investigation have successfully evaluated the instrument's first images, revealing the speed and temperature of material flowing out from the sun. ...

Advanced orbital constellations for solar storm defense

Solar storms have the potential to cause catastrophic damage. One that occurred around the end of October 2003 (now called the 2003 Halloween Storm) caused an estimated $27B in damages. That number will only increase as humanity ...

Is the world ready for a catastrophic solar storm?

Some 13,000 years ago, the sun emitted a huge belch of radiation that bombarded Earth and left its imprint in ancient tree rings. That solar storm was the most powerful one ever recorded. The next strongest was the 1859 Carrington ...

Space weather can dramatically alter a planet's fate

We tend to think of habitability in terms of individual planets and their potential to host life. But barring outliers like rogue planets with internal heating or icy moons with subsurface oceans created by tidal heating, ...

page 6 from 10