The gigantic coronal hole is blasting high-speed solar wind toward Earth, potentially igniting vibrant auroras and minor geomagnetic activity on Jan. 31.
First proposed in the 1950s by University of Chicago physicist Eugene Parker, the solar wind is visible in the halo around the sun during an eclipse and sometimes when the particles hit the Earth’s ...
Atmospheric Motion Vectors (AMVs) are crucial for understanding wind patterns and dynamics in the atmosphere. They are derived from satellite imagery that captures the movement of clouds and water ...