Solar coronal shocks often produce Type II solar radio bursts, also known as slow-drifting bursts, which travel outward from the Sun at speeds of around 1,000 km per second.
occur around solar maximum, the most active portion of the Sun’s 11 year cycle. One such maximum was recently passed, but ...
Researchers delving into solar coronal shocks triggered by solar flares have cracked a long-standing puzzle about the reason behind the strange variation in the relative strengths of radio waves ...
The study improves scientists’ understanding of how solar shocks generate radio waves and how those waves travel through the ...
A study published today in Nature Astronomy examines solar radio aurora observed almost 25,000 miles (40,000 kilometers) above sunspots using the New Jersey Institute of Technology’s Center for ...
Antennas installed at 18 U.S. high schools detected bursts of radio activity that can precede solar disturbances capable of disrupting satellites and power grids on Earth. The observations helped ...
Some results have been hidden because they may be inaccessible to you
Show inaccessible results