Due to most of the regions on the solar disk being fairly simple in
their magnetic complexity, solar activity is expected to remain at
low levels with a chance for M-class flares (R1 to R2, or Minor to
Moderate).
Solar wind parameters are expected to trend further towards nominal
levels as the Coronal Hole High-Speed Stream effects continue to
wane.
Additional enhancements from another negative polari…
Read more
American Radio Relay League | Ham Radio Association and Resources – Read More
More Stories
via Hackaday: Keep Bears at Bay with the Crackle of 280,000 Volts
via Amateur Radio Daily: Webinar Tonight: IP400 and The Digital Future of Amateur Radio
via the ARRL: ARRL Iowa Section Wins Ham Exemption to Handsfree Law